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"url": "https://datacentral.org.au/api/schema/2/",
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"description": "<p>DEVILS is a spectroscopic campaign at the Anglo-Australian Telescope aimed at bridging the near and distant Universe by producing the highest completeness survey of galaxies and groups at intermediate redshifts (0.3<z<1.0). Our sample will consist of ~58k galaxies to Ymag<21.2, over ~6deg<sup>2</sup> to >95% completeness in three well studies deep extragalactic fields (COSMOS, ECDFS and XMM-LSS).</p>",
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"documentation": "ApMatchedPhotom<br>ApMatchedCat<br>v02<br>2012-04-23<br>Mehmet Alpaslan <mehmet.alpaslan@icrar.org><br><br>This catalogue provides Kron and Petrosian photometry for all GAMA DR2<br>objects, as well as other Source Extractor outputs for the ugrizYJHK<br>bands obtained from the v02 mosaics using <a href=\"http://www.astromatic.net/software/sextractor\">Source Extractor</a>.<br><br>The GAMA mosaics have been constructed by stitching together<br>individual frames of images taken from the SDSS and UKIDSS LAS surveys<br>using <a href=\"http://www.astromatic.net/software/swarp\">SWarp</a>, a resampling and co-adding program. There is one mosaic<br>per band and per GAMA survey region. All frames in the mosaics have<br>been pre-convolved to a common seeing of 2 arcsec and renormalised.<br>The pixel scale of these mosaics (and hence of the present catalogue)<br>is 0.339 arcsec per pixel. The zero-point used throughout is 30 mag.<br>The mosaics are available on the <a href=\"/dr2/data/imaging/gama/mosaics/v02/\">DR2 file server</a> (swpci* files).<br><br>The photometry was obtained by using Source Extractor in matched<br>aperture mode. In short, this mode allows Source Extractor to fit an<br>aperture around a possible source in one image, and measure the flux<br>from another. In the present case, we have fit the apertures to r-band<br>images and measure the fluxes in all 9 bands. This process was<br>automated using a wrapper written in <a href=\"http://www.r-project.org/\">R</a> that creates a cutout image of<br>each source in all 9 bands, each of which is fed into Source Extractor<br>alongside the master r-band cutout. Where Source Extractor fails to<br>calculate a magnitude (for whatever reason) the default value returned<br>is 99. Any nonsense results (negative values for FLUX, BACKGROUND or<br>FWHM) are caused by Source Extractor failing; in these cases consult<br>the appropriate FLAGS column to get some indication as to why this is<br>happening.<br><br>Some small areas of the GAMA survey regions are not covered by the<br>YJHK mosaics because some frames in these bands had to be removed due<br>to poor image quality. The YJHK magnitudes and errors of objects<br>located in these areas have been set to -99, while their fluxes and<br>associated errors have been set to 0 and 1E99, respectively.<br><br>#######################################################################<br><br>MAG_AUTO_ / MAG_PETRO_<br><br>The magnitudes presented in this catalogue have not been corrected for<br>the effect of foreground Milky Way dust extinction. Should these<br>corrections be required, they can be obtained from the table<br>GalacticExtinction in the InputCat DMU.<br><br>All photomotry is on the AB system.<br><br>#######################################################################<br><br>Photometric errors<br><br>The errors associated with the MAG_AUTO and MAG_PETRO values have been<br>calculated and rescaled in such a way as to match the errors used in<br>the SDSS and UKIDSS photometry catalogues. To do this, the raw Source<br>Extractor errors have been taken and, for each band, rescaled such<br>that they match these existing photometry catalogues as accurately as<br>possible. The original Source Extractor errors are preserved in the<br>_SE columns.<br><br>########################################################################<br><br>Potential zero-point offsets<br><br>From recent comparisons with VIKING and 2MASS we have discovered an<br>apparent zero-point offset in our photometry derived from the UKIDSS<br>LAS data. The cause of this offset is still not fully understood.<br>This issue will be described in more detail in a future paper<br>presenting the GAMA II panchromatic photometry catalogue (Driver et<br>al., in prep.). 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In this case, these are not used.<br><br>PHOT_FLUXFRAC\t\t0.5\t<br>Fraction of flux used to determine each element of the flux radius vector.<br><br>SATUR_LEVEL\t\t500000\t<br>Pixel value above which the pixel is considered saturated. <br><br>MAG_ZEROPOINT\t\t30<br>Zero-point offset applied to magnitudes.<br><br>PIXEL_SCALE\t\t0.339\t<br>Pixel scale in arcsec.<br><br>For a detailed explanation of what each of these parameters does,<br>please see this third party <a href=\"http://astro.dur.ac.uk/~pdraper/extractor/Guide2source_extractor.pdf\">guide to Source Extractor</a>.<br><br>",
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},
{
"id": 5,
"name": "EnvironmentMeasures",
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"documentation": "EnvironmentMeasures<br>EnvironmentMeasures<br>v02<br>2014-08-21<br>Sarah Brough <sb@aao.gov.au><br><br>The EnvironmentMeasures DMU provides several different metrics of the<br>local environment of GAMA DR2 galaxies: a surface density, the number<br>of galaxies within a cylinder, and the density of galaxies within an<br>adaptive Gaussian ellipsoid. <br><br>Note that this release only covers the GAMA G15 survey region.<br><br>All of these environment measurements are performed on a density<br>defining pseudo-volume-limited population of galaxies. This population<br>is defined as all galaxies with M_r(z_ref=0, Q=0.78) < -20.4 mag,<br>where Q defines the expected evolution of M_r as a function of<br>redshift. Q is taken from Loveday et al. (2014, in prep). Given the<br>depth of the GAMA I survey (r < 19.4 mag) the above absolute magnitude<br>limit implies a redshift (i.e. volume) limit of z=0.18333. However, in<br>order to account for the upper edge of the velocity range employed<br>when searching for nearby galaxies (see below), the environment<br>measurements are only provided for galaxies out to z=0.18. The exact<br>sample included in this DMU is: all GAMA DR2 galaxies in G15 with<br>redshift quality nQ > 2 (i.e. reliable redshifts) and within the<br>redshift limits of 0.002 < Z_TONRY <= 0.18.<br><br>This catalogue is based on DistancesFrames (which is itself based on<br>TilingCat), kCorrections and the GAMA I final completeness masks, and<br>uses H_0 = 70 km/s/Mpc, O_M = 0.3, O_L = 0.7.<br><br>#######################################################################<br><br>IMPORTANT NOTE:<br><br>On 2014-09-03 this DMU was upgraded from v01 to v02 following the<br>discovery of two bugs in v01. In v01 the faint limit of the density<br>defining population was incorrectly set to -20 mag. It has now been<br>set to the correct value of -20.4 mag. There was also a bug in the<br>flagging of galaxies. We furthermore took the opportunity to update<br>the value of Q from 0.87 (v01) to 0.78 (v02).<br><br>#######################################################################<br><br>We now describe the three environment measures provided by this DMU in<br>more detail.<br><br>SurfaceDensity:<br>This column provides the surface density based on the distance to the<br>5th nearest neighbour among the density defining population in a<br>velocity cylinder of +/-1000 km/s, i.e. 5 / (Pi * DistanceTo5nn^2).<br><br>CountInCyl:<br>This column provides the number of (other) galaxies from the density<br>defining population within a cylinder of co-moving radius 1 Mpc and a<br>velocity range of +/-1000 km/s. The overdensity is given by<br>CountInCyl / (nbar_ref * volume_of_cylinder)<br>where nbar_ref = 0.00703 Mpc^-3 is the average number density of the<br>density defining population. <br><br>AGEDensity:<br>This column provides the density of galaxies from the density defining<br>population in an adaptive Gaussian ellipsoid defined by<br>(r_a/(3*sigma))^2 + (r_z/(3*AGEScale*sigma))^2 <= 1, where r_a and r_z<br>are the distances from the centre in the plane of sky and along the<br>line-of-sight in co-moving Mpc, respectively, and sigma = 2 Mpc. The<br>adaptive scaling factor, AGEScale = 1 + (0.2*n_gals_within_2Mpc), is<br>used to scale the value of sigma along the redshift axis by up to a<br>factor of 3 (i.e. n_gals_within_2Mpc[max]=10) for the highest density<br>environments to compensate for the \"finger-of-God\" effect (<a href=\"http://adsabs.harvard.edu/abs/2007ApJS..173..512S\">Schawinski<br>et al. (2007)</a>, <a href=\"http://adsabs.harvard.edu/abs/2010MNRAS.404.1775T\">Thomas et al. (2010)</a>).<br><br>#######################################################################<br><br>All unflagged environment measures are corrected for survey<br>incompleteness as (for example):<br>SurfaceDensity = SurfaceDensity_raw * (1 / Completeness),<br>where Completeness is the local completeness as given by the<br>completeness mask at the position of the galaxy, and not a completeness<br>averaged over the area or volume over which the environment measure is<br>determined.<br><br>#######################################################################<br><br>The errors on the environment measures are calculated as follows.<br><br>SurfaceDensityErr:<br>Calculated as the larger of <br>|(SurfaceDensity to 5th nearest neighbour) -<br> (SurfaceDensity to 4th nearest neighbour)| <br>and<br>|(SurfaceDensity to 5th nearest neighbour) - <br> (SurfaceDensity to 6th nearest neighbour)|<br><br>CountInCylErr:<br>Calculated as sqrt(CountInCyl).<br><br>AGEErr:<br>Calculated as sqrt(Ngals).<br>Note that this is the Poisson error on the number of galaxies found in<br>the adaptive Gaussian ellipsoid. It is *not* the error on AGEDensity.<br><br>#######################################################################<br><br>Below we describe the meanings of the various problem-indicating flags.<br><br>SurfaceDensityFlag:<br><br> Flag value Flag meaning<br> ------------------------------------------------------------------<br> 0 SurfaceDensity is exact.<br> 1 The distance to the 5th nearest neighbour is larger<br> than the distance to the nearest angular survey<br> edge, but a nearer galaxy is within this distance.<br> The surface density is calculated using the<br> distance to the nearer galaxy and hence<br> SurfaceDensity is an upper limit.<br> 2 No neighbours found among the density defining<br> population within the distance to the nearest<br> angular survey edge. SurfaceDensity is calculated<br> as 1 / (Pi * DistanceToEdge^2).<br> 4 The galaxy lies inside a bright star exclusion<br> region (Completeness=-1) or outside of the GAMA<br> survey boundary (as defined by the completeness<br> mask, Completeness=-2). SurfaceDensity cannot be<br> determined accurately and is set to -999.9.<br><br><br>CountInCylFlag:<br><br> Flag value Flag meaning<br> ------------------------------------------------------------------<br> 0 CountInCyl is exact.<br> 1 The cylinder extends across the nearest angular<br> survey edge. CountInCyl is a lower limit.<br> 2 The galaxy lies inside a bright star exclusion<br> region (Completeness=-1) or outside of the GAMA<br> survey boundary (as defined by the completeness<br> mask, Completeness=-2). CountInCyl cannot be <br> determined accurately and is set to -999.9.<br><br><br>AGEDensityFlag:<br><br> Flag value Flag meaning<br> ------------------------------------------------------------------<br> 0 AGEDensity is exact.<br> 1 The ellipsoid extends across the nearest angular<br> survey edge. AGEDensity is set to -999.9.<br> 2 No (other) galaxies from the density defining<br> population are found within the ellipsoid (not due<br> to angular survey edge). AGEDensity is set to<br> -999.9.<br> 4 The galaxy lies inside a bright star exclusion<br> region (Completeness=-1) or outside of the GAMA<br> survey boundary (as defined by the completeness<br> mask, Completeness=-2). AGEDensity cannot be <br> determined accurately and is set to -999.9.<br><br>#######################################################################<br><br>M_r:<br>Calculated as R_PETRO - Dmod70 - KCOR_(r,zref=0).<br><br>",
"file_path": null,
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"version": "v02",
"type": "CatalogueGroup",
"created": "2021-01-28T00:39:52.881517Z",
"updated": "2021-02-09T04:07:34.424417Z",
"contact": {
"email": "sb@aao.gov.au",
"name": "Sarah Brough "
},
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{
"id": 5,
"name": "EnvironmentMeasures",
"pretty_name": null,
"description": "This catalogue provides three different environment measures for all GAMA DR2 galaxies in G15 with 0.002 < z < 0.18: a surface density, the number of galaxies within a cylinder, and the density of galaxies within an adaptive Gaussian ellipsoid.",
"documentation": "EnvironmentMeasures<br>EnvironmentMeasures<br>v02<br>2014-08-21<br>Sarah Brough <sb@aao.gov.au><br><br>The EnvironmentMeasures DMU provides several different metrics of the<br>local environment of GAMA DR2 galaxies: a surface density, the number<br>of galaxies within a cylinder, and the density of galaxies within an<br>adaptive Gaussian ellipsoid. <br><br>Note that this release only covers the GAMA G15 survey region.<br><br>All of these environment measurements are performed on a density<br>defining pseudo-volume-limited population of galaxies. This population<br>is defined as all galaxies with M_r(z_ref=0, Q=0.78) < -20.4 mag,<br>where Q defines the expected evolution of M_r as a function of<br>redshift. Q is taken from Loveday et al. (2014, in prep). Given the<br>depth of the GAMA I survey (r < 19.4 mag) the above absolute magnitude<br>limit implies a redshift (i.e. volume) limit of z=0.18333. However, in<br>order to account for the upper edge of the velocity range employed<br>when searching for nearby galaxies (see below), the environment<br>measurements are only provided for galaxies out to z=0.18. The exact<br>sample included in this DMU is: all GAMA DR2 galaxies in G15 with<br>redshift quality nQ > 2 (i.e. reliable redshifts) and within the<br>redshift limits of 0.002 < Z_TONRY <= 0.18.<br><br>This catalogue is based on DistancesFrames (which is itself based on<br>TilingCat), kCorrections and the GAMA I final completeness masks, and<br>uses H_0 = 70 km/s/Mpc, O_M = 0.3, O_L = 0.7.<br><br>#######################################################################<br><br>IMPORTANT NOTE:<br><br>On 2014-09-03 this DMU was upgraded from v01 to v02 following the<br>discovery of two bugs in v01. In v01 the faint limit of the density<br>defining population was incorrectly set to -20 mag. It has now been<br>set to the correct value of -20.4 mag. There was also a bug in the<br>flagging of galaxies. We furthermore took the opportunity to update<br>the value of Q from 0.87 (v01) to 0.78 (v02).<br><br>#######################################################################<br><br>We now describe the three environment measures provided by this DMU in<br>more detail.<br><br>SurfaceDensity:<br>This column provides the surface density based on the distance to the<br>5th nearest neighbour among the density defining population in a<br>velocity cylinder of +/-1000 km/s, i.e. 5 / (Pi * DistanceTo5nn^2).<br><br>CountInCyl:<br>This column provides the number of (other) galaxies from the density<br>defining population within a cylinder of co-moving radius 1 Mpc and a<br>velocity range of +/-1000 km/s. The overdensity is given by<br>CountInCyl / (nbar_ref * volume_of_cylinder)<br>where nbar_ref = 0.00703 Mpc^-3 is the average number density of the<br>density defining population. <br><br>AGEDensity:<br>This column provides the density of galaxies from the density defining<br>population in an adaptive Gaussian ellipsoid defined by<br>(r_a/(3*sigma))^2 + (r_z/(3*AGEScale*sigma))^2 <= 1, where r_a and r_z<br>are the distances from the centre in the plane of sky and along the<br>line-of-sight in co-moving Mpc, respectively, and sigma = 2 Mpc. The<br>adaptive scaling factor, AGEScale = 1 + (0.2*n_gals_within_2Mpc), is<br>used to scale the value of sigma along the redshift axis by up to a<br>factor of 3 (i.e. n_gals_within_2Mpc[max]=10) for the highest density<br>environments to compensate for the \"finger-of-God\" effect (<a href=\"http://adsabs.harvard.edu/abs/2007ApJS..173..512S\">Schawinski<br>et al. (2007)</a>, <a href=\"http://adsabs.harvard.edu/abs/2010MNRAS.404.1775T\">Thomas et al. (2010)</a>).<br><br>#######################################################################<br><br>All unflagged environment measures are corrected for survey<br>incompleteness as (for example):<br>SurfaceDensity = SurfaceDensity_raw * (1 / Completeness),<br>where Completeness is the local completeness as given by the<br>completeness mask at the position of the galaxy, and not a completeness<br>averaged over the area or volume over which the environment measure is<br>determined.<br><br>#######################################################################<br><br>The errors on the environment measures are calculated as follows.<br><br>SurfaceDensityErr:<br>Calculated as the larger of <br>|(SurfaceDensity to 5th nearest neighbour) -<br> (SurfaceDensity to 4th nearest neighbour)| <br>and<br>|(SurfaceDensity to 5th nearest neighbour) - <br> (SurfaceDensity to 6th nearest neighbour)|<br><br>CountInCylErr:<br>Calculated as sqrt(CountInCyl).<br><br>AGEErr:<br>Calculated as sqrt(Ngals).<br>Note that this is the Poisson error on the number of galaxies found in<br>the adaptive Gaussian ellipsoid. It is *not* the error on AGEDensity.<br><br>#######################################################################<br><br>Below we describe the meanings of the various problem-indicating flags.<br><br>SurfaceDensityFlag:<br><br> Flag value Flag meaning<br> ------------------------------------------------------------------<br> 0 SurfaceDensity is exact.<br> 1 The distance to the 5th nearest neighbour is larger<br> than the distance to the nearest angular survey<br> edge, but a nearer galaxy is within this distance.<br> The surface density is calculated using the<br> distance to the nearer galaxy and hence<br> SurfaceDensity is an upper limit.<br> 2 No neighbours found among the density defining<br> population within the distance to the nearest<br> angular survey edge. SurfaceDensity is calculated<br> as 1 / (Pi * DistanceToEdge^2).<br> 4 The galaxy lies inside a bright star exclusion<br> region (Completeness=-1) or outside of the GAMA<br> survey boundary (as defined by the completeness<br> mask, Completeness=-2). SurfaceDensity cannot be<br> determined accurately and is set to -999.9.<br><br><br>CountInCylFlag:<br><br> Flag value Flag meaning<br> ------------------------------------------------------------------<br> 0 CountInCyl is exact.<br> 1 The cylinder extends across the nearest angular<br> survey edge. CountInCyl is a lower limit.<br> 2 The galaxy lies inside a bright star exclusion<br> region (Completeness=-1) or outside of the GAMA<br> survey boundary (as defined by the completeness<br> mask, Completeness=-2). CountInCyl cannot be <br> determined accurately and is set to -999.9.<br><br><br>AGEDensityFlag:<br><br> Flag value Flag meaning<br> ------------------------------------------------------------------<br> 0 AGEDensity is exact.<br> 1 The ellipsoid extends across the nearest angular<br> survey edge. AGEDensity is set to -999.9.<br> 2 No (other) galaxies from the density defining<br> population are found within the ellipsoid (not due<br> to angular survey edge). AGEDensity is set to<br> -999.9.<br> 4 The galaxy lies inside a bright star exclusion<br> region (Completeness=-1) or outside of the GAMA<br> survey boundary (as defined by the completeness<br> mask, Completeness=-2). AGEDensity cannot be <br> determined accurately and is set to -999.9.<br><br>#######################################################################<br><br>M_r:<br>Calculated as R_PETRO - Dmod70 - KCOR_(r,zref=0).<br><br>",
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"created": "2021-01-28T00:39:53.325772Z",
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"contact": {
"email": "sb@aao.gov.au",
"name": "Sarah Brough "
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"description": "Extinction and k-corrected absolute r-band magnitude",
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"description": "This DMU collects spectra for GAMA DR2 objects from previous spectroscopic surveys such as the SDSS.",
"documentation": "ExternalSpec<br>2011-03-03<br>Joe Liske <jliske@eso.org><br><br>The ExternalSpec DMU collects spectra of GAMA DR2 objects from<br>existing spectroscopic surveys. The spectra were taken from the<br>following surveys:<br><br> Survey\t # of spectra<br> ------------------------------------------------<br> SDSS\t\tDR7\t\t 16267<br> 2dFGRS\tFinal data release 11906<br> 2QZ\t\tFinal data release 150<br> MGC\t\tFinal data release 2154<br> 2SLAQ-LRG\tFinal data release 44<br> 2SLAQ-QSO\tFinal data release 43<br> WiggleZ\tDR1\t\t 16<br> 6dFGS\tFinal data release 248<br> ------------------------------------------------<br> Total\t 30828<br><br>Duplicate observations have been included (except in the case of<br>WiggleZ). The spectra are provided as 1D fits files and are available<br>from the <a href=\"/dr2/data/\">GAMA DR2 fileserver</a> in the directory spectra/. The files are<br>essentially those that are provided by the various surveys, except<br>that multiple extensions (sometimes used to store duplicate<br>observations) are extracted to individual files. For each spectrum we<br>have also added its entry from the ExternalSpecAll table (see below)<br>to the fits header. In case of conflicts with existing keywords, these<br>were first renamed.<br><br>See the directory descriptions for the various survey data on the GAMA<br>fileserver for more details.<br><br>-----------------------------------------------------------------------<br><br>Apart from the spectra, this DMU also produces the table<br>ExternalSpecAll, which lists all of the available external spectra<br>(including all duplicate observations) as well as their redshifts as<br>determined by the originating surveys. In addition, the table<br>ExternalSpec is provided, which lists only the those external spectra<br>that provide the best redshifts for GAMA DR2 objects. Both are in the<br>same format and the latter is an exact subset of the former. In fact,<br>ExternalSpec is a \"view\" of ExternalSpecAll. It lists only those<br>entries with IS_SBEST = TRUE, meaning that it excludes intra-survey<br>duplicate observations. However, it still includes inter-survey<br>duplications.<br><br>In the following we provide additional information for some of the<br>parameters in these tables:<br><br>SPECID: <br>-------<br>This is the spectrum's unique identifier as used in the GAMA DR2<br>database. The value of this parameter depends on the orginating survey<br>of the spectrum:<br><br> SDSS:\tspecObjID<br> 2dFGRS: \"2dF\"SEQNUM (+ _n for duplications, where n=2,3,4)<br> 2QZ: \"2QZ\"IAUNAMEx (where x=a,b,c,d,e,f)<br> MGC:\t \t\"MGC\"ID (+ _n for duplications, where n=2,3,4,5)<br> 2SLAQ-LRG: \"2SL\"IAUNAME_n (where n=1,2,3,4)<br> 2SLAQ-QSO:\t\"2SL\"IAUNAME_FLD_DATE<br> WiggleZ: \t\"W\"n (where n is a multi-digit number taken from the file name)<br> 6dFGS: \t\"6dF\"TARGETNAME (+ _n for duplications, n=2)<br><br><br>nQ:<br>---<br>This is a redshift quality flag. We have attempted to translate the<br>redshift qualities of the various surveys to the GAMA system (nQ =<br>0-4, with nQ >= 3 used for science):<br><br>SDSS:<br>nQ = 1 + (zconf > 0.2) + (zwarning_ok && zconf > 0.7) + <br> (zconf > 0.9) + (zconf > 0.99) <br>where zwarning_ok is 1 if there are no absorption or emission line<br>redshift inconsistencies and the 4000 A break is not too large.<br>Note that in the case of the SDSS we allow nQ = 5 because of the<br>exceptional reliability of these redshifts.<br><br>2dFGRS:<br>If QUALITY = 5 then nQ = 4, else nQ = QUALITY.<br><br>2QZ:<br> nQ QUALTHIS<br> -------------------<br> 3 11<br> 2 12,21,22<br> 1 23,33<br><br>MGC:<br>If Z_QUAL = 5 then nQ = 4, else nQ = Z_QUAL.<br><br>2SLAQ-LRG:<br>If qop >= 3 then nQ = 3, else nQ = qop.<br><br>2SLAQ-QSO:<br> nQ qual<br> -------------------<br> 3 11<br> 2 12,21,22<br> 1 23,33<br><br>WiggleZ:<br>If Qop >= 3 then nQ = 3, else nQ = Qop.<br><br>6dFGS:<br>If QUALITY >= 3 then nQ = 3, else nQ = QUALITY.<br><br><br>PROB:<br>-----<br>This parameter is set to zconf for spectra from the SDSS, and to 0 in<br>all other cases.<br><br><br>CATAID / GAMA_NAME:<br>-------------------<br>These parameters identify the GAMA object the spectrum was matched to.<br>For a given spectrum a matching GAMA object was identified by finding<br>the spectrum's closest GAMA object (within 2 arcsec) in the catalogue<br>resulting from the union of TilingCat and SpStandards from the<br><a href=\"/dr2/schema/dmu.php?name=InputCat\">InputCat DMU</a>.<br><br><br>IC_FLAG:<br>--------<br>This is a bitwise flag identifying the catalogue(s) in which the<br>matched GAMA object was found:<br><br> Bit n 2^(n-1) Catalogue<br> ------------------------------<br> 1 1 InputCatA\t<br> 2 2 TilingCat<br> 3 4 SpStandards<br><br><br>DIST:<br>-----<br>Distance between the spectrum and the matched GAMA object in arcsec.<br><br><br>IS_SBEST:<br>---------<br>In cases where multiple spectra from a given survey were matched to<br>the same GAMA object this flag identifies the spectrum that provides<br>the best redshift for that object.<br><br>SDSS:<br>The spectrum providing the best redshift was identified by first<br>considering only sciencePrimary spectra with nQ >= 3 and within 1<br>arcsec of the object. If there were multiple, then we selected the one<br>with the highest nQ value. If there were multiple with the same nQ<br>value, we selected the closest spectrum. In cases without any nQ >= 3<br>sciencePrimary spectra within 1 arcsec we simply selected first by nQ,<br>then by distance.<br><br>All other surveys:<br>The spectrum providing the best redshift was selected first by nQ, and<br>then (in cases of multiple spectra with the same nQ) by distance<br>between the object and the spectrum.<br><br>-----------------------------------------------------------------------<br><br>This DMU also provides the table ExternalzAll which contains a<br>relatively small number of redshifts from various literature sources,<br>where the original spectra from which these redshifts were measured<br>are not available to GAMA.<br><br>Redshifts have been collected from the following sources:<br><br> Survey\t\t\t# of redshifts\tSource<br> ---------------------------------------------------------------------<br> NED\t\t\t\t 3\t\tNED website<br> Updated Zwicky Catalog\t214\t\tVizieR: J/PASP/111/438<br> ---------------------------------------------------------------------<br> Total\t\t\t217<br><br>All redshifts were matched to GAMA objects in the same way as the<br>spectra above.<br><br><br>SPECID: <br>-------<br> NED:\t\t\"NED_\"common_name<br> UZC: \t\"UZC\"serial_number<br><br><br>nQ and PROB:<br>------------<br> NED:\t\tnQ = 3<br>\t PROB = 0.0<br> UZC:\t\tnQ = 3 if UZC_class = 0 or 1, else nQ = 2<br>\t\tPROB = 0.0<br><br>",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v01",
"type": "CatalogueGroup",
"created": "2021-01-28T00:39:52.918641Z",
"updated": "2021-02-09T04:07:34.439620Z",
"contact": {
"email": "jliske@eso.org",
"name": "Joe Liske "
},
"tables": [
{
"id": 6,
"name": "ExternalSpec",
"pretty_name": null,
"description": "This table lists those spectra from previous spectroscopic surveys (such as the SDSS) that provide the best redshifts for GAMA DR2 objects. This table is an exact subset of the table ExternalSpecAll. It lists only those entries with IS_SBEST = TRUE, meaning that it excludes intra-survey duplicate observations. However, it still includes inter-survey duplications.",
"documentation": "ExternalSpec<br>2011-03-03<br>Joe Liske <jliske@eso.org><br><br>The ExternalSpec DMU collects spectra of GAMA DR2 objects from<br>existing spectroscopic surveys. The spectra were taken from the<br>following surveys:<br><br> Survey\t # of spectra<br> ------------------------------------------------<br> SDSS\t\tDR7\t\t 16267<br> 2dFGRS\tFinal data release 11906<br> 2QZ\t\tFinal data release 150<br> MGC\t\tFinal data release 2154<br> 2SLAQ-LRG\tFinal data release 44<br> 2SLAQ-QSO\tFinal data release 43<br> WiggleZ\tDR1\t\t 16<br> 6dFGS\tFinal data release 248<br> ------------------------------------------------<br> Total\t 30828<br><br>Duplicate observations have been included (except in the case of<br>WiggleZ). The spectra are provided as 1D fits files and are available<br>from the <a href=\"/dr2/data/\">GAMA DR2 fileserver</a> in the directory spectra/. The files are<br>essentially those that are provided by the various surveys, except<br>that multiple extensions (sometimes used to store duplicate<br>observations) are extracted to individual files. For each spectrum we<br>have also added its entry from the ExternalSpecAll table (see below)<br>to the fits header. In case of conflicts with existing keywords, these<br>were first renamed.<br><br>See the directory descriptions for the various survey data on the GAMA<br>fileserver for more details.<br><br>-----------------------------------------------------------------------<br><br>Apart from the spectra, this DMU also produces the table<br>ExternalSpecAll, which lists all of the available external spectra<br>(including all duplicate observations) as well as their redshifts as<br>determined by the originating surveys. In addition, the table<br>ExternalSpec is provided, which lists only the those external spectra<br>that provide the best redshifts for GAMA DR2 objects. Both are in the<br>same format and the latter is an exact subset of the former. In fact,<br>ExternalSpec is a \"view\" of ExternalSpecAll. It lists only those<br>entries with IS_SBEST = TRUE, meaning that it excludes intra-survey<br>duplicate observations. However, it still includes inter-survey<br>duplications.<br><br>In the following we provide additional information for some of the<br>parameters in these tables:<br><br>SPECID: <br>-------<br>This is the spectrum's unique identifier as used in the GAMA DR2<br>database. The value of this parameter depends on the orginating survey<br>of the spectrum:<br><br> SDSS:\tspecObjID<br> 2dFGRS: \"2dF\"SEQNUM (+ _n for duplications, where n=2,3,4)<br> 2QZ: \"2QZ\"IAUNAMEx (where x=a,b,c,d,e,f)<br> MGC:\t \t\"MGC\"ID (+ _n for duplications, where n=2,3,4,5)<br> 2SLAQ-LRG: \"2SL\"IAUNAME_n (where n=1,2,3,4)<br> 2SLAQ-QSO:\t\"2SL\"IAUNAME_FLD_DATE<br> WiggleZ: \t\"W\"n (where n is a multi-digit number taken from the file name)<br> 6dFGS: \t\"6dF\"TARGETNAME (+ _n for duplications, n=2)<br><br><br>nQ:<br>---<br>This is a redshift quality flag. We have attempted to translate the<br>redshift qualities of the various surveys to the GAMA system (nQ =<br>0-4, with nQ >= 3 used for science):<br><br>SDSS:<br>nQ = 1 + (zconf > 0.2) + (zwarning_ok && zconf > 0.7) + <br> (zconf > 0.9) + (zconf > 0.99) <br>where zwarning_ok is 1 if there are no absorption or emission line<br>redshift inconsistencies and the 4000 A break is not too large.<br>Note that in the case of the SDSS we allow nQ = 5 because of the<br>exceptional reliability of these redshifts.<br><br>2dFGRS:<br>If QUALITY = 5 then nQ = 4, else nQ = QUALITY.<br><br>2QZ:<br> nQ QUALTHIS<br> -------------------<br> 3 11<br> 2 12,21,22<br> 1 23,33<br><br>MGC:<br>If Z_QUAL = 5 then nQ = 4, else nQ = Z_QUAL.<br><br>2SLAQ-LRG:<br>If qop >= 3 then nQ = 3, else nQ = qop.<br><br>2SLAQ-QSO:<br> nQ qual<br> -------------------<br> 3 11<br> 2 12,21,22<br> 1 23,33<br><br>WiggleZ:<br>If Qop >= 3 then nQ = 3, else nQ = Qop.<br><br>6dFGS:<br>If QUALITY >= 3 then nQ = 3, else nQ = QUALITY.<br><br><br>PROB:<br>-----<br>This parameter is set to zconf for spectra from the SDSS, and to 0 in<br>all other cases.<br><br><br>CATAID / GAMA_NAME:<br>-------------------<br>These parameters identify the GAMA object the spectrum was matched to.<br>For a given spectrum a matching GAMA object was identified by finding<br>the spectrum's closest GAMA object (within 2 arcsec) in the catalogue<br>resulting from the union of TilingCat and SpStandards from the<br><a href=\"/dr2/schema/dmu.php?name=InputCat\">InputCat DMU</a>.<br><br><br>IC_FLAG:<br>--------<br>This is a bitwise flag identifying the catalogue(s) in which the<br>matched GAMA object was found:<br><br> Bit n 2^(n-1) Catalogue<br> ------------------------------<br> 1 1 InputCatA\t<br> 2 2 TilingCat<br> 3 4 SpStandards<br><br><br>DIST:<br>-----<br>Distance between the spectrum and the matched GAMA object in arcsec.<br><br><br>IS_SBEST:<br>---------<br>In cases where multiple spectra from a given survey were matched to<br>the same GAMA object this flag identifies the spectrum that provides<br>the best redshift for that object.<br><br>SDSS:<br>The spectrum providing the best redshift was identified by first<br>considering only sciencePrimary spectra with nQ >= 3 and within 1<br>arcsec of the object. If there were multiple, then we selected the one<br>with the highest nQ value. If there were multiple with the same nQ<br>value, we selected the closest spectrum. In cases without any nQ >= 3<br>sciencePrimary spectra within 1 arcsec we simply selected first by nQ,<br>then by distance.<br><br>All other surveys:<br>The spectrum providing the best redshift was selected first by nQ, and<br>then (in cases of multiple spectra with the same nQ) by distance<br>between the object and the spectrum.<br><br>-----------------------------------------------------------------------<br><br>This DMU also provides the table ExternalzAll which contains a<br>relatively small number of redshifts from various literature sources,<br>where the original spectra from which these redshifts were measured<br>are not available to GAMA.<br><br>Redshifts have been collected from the following sources:<br><br> Survey\t\t\t# of redshifts\tSource<br> ---------------------------------------------------------------------<br> NED\t\t\t\t 3\t\tNED website<br> Updated Zwicky Catalog\t214\t\tVizieR: J/PASP/111/438<br> ---------------------------------------------------------------------<br> Total\t\t\t217<br><br>All redshifts were matched to GAMA objects in the same way as the<br>spectra above.<br><br><br>SPECID: <br>-------<br> NED:\t\t\"NED_\"common_name<br> UZC: \t\"UZC\"serial_number<br><br><br>nQ and PROB:<br>------------<br> NED:\t\tnQ = 3<br>\t PROB = 0.0<br> UZC:\t\tnQ = 3 if UZC_class = 0 or 1, else nQ = 2<br>\t\tPROB = 0.0<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/ExternalSpec.fits",
"file_name": "ExternalSpec.fits",
"file_extension": "fits",
"version": "v01",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.372911Z",
"updated": "2021-02-09T04:07:34.632782Z",
"contact": {
"email": "jliske@eso.org",
"name": "Joe Liske "
},
"input_cat": false,
"columns": [
{
"id": 197,
"name": "CATAID",
"pretty_name": null,
"description": "ID of matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:39:59.848237Z",
"updated": "2021-02-09T04:07:37.682027Z",
"contact": null,
"ucd": "meta.id.cross;src",
"unit": "-"
},
{
"id": 198,
"name": "DEC",
"pretty_name": null,
"description": "DEC of spectrum (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:39:59.881248Z",
"updated": "2021-02-09T04:07:37.693812Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 199,
"name": "DIST",
"pretty_name": null,
"description": "Distance between spectrum and matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:39:59.913962Z",
"updated": "2021-02-09T04:07:37.706002Z",
"contact": null,
"ucd": "pos.angDistance",
"unit": "arcsec"
},
{
"id": 200,
"name": "FILENAME",
"pretty_name": null,
"description": "Full path and filename of the spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:39:59.939491Z",
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"contact": null,
"ucd": "meta.id;meta.file;meta.fits",
"unit": "-"
},
{
"id": 201,
"name": "GAMA_NAME",
"pretty_name": null,
"description": "Name of matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:39:59.965125Z",
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},
{
"id": 202,
"name": "IC_FLAG",
"pretty_name": null,
"description": "Catalogue source(s) of matched GAMA object",
"documentation": "",
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"file_name": null,
"file_extension": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:39:59.999713Z",
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},
{
"id": 203,
"name": "IS_SBEST",
"pretty_name": null,
"description": "Is this the spectrum with the best redshift of this GAMA object within the originating survey?",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.034936Z",
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},
{
"id": 204,
"name": "NQ",
"pretty_name": null,
"description": "Normalised redshift quality (use nQ > 2 for science)",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.055829Z",
"updated": "2021-02-09T04:07:37.767650Z",
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"unit": "-"
},
{
"id": 205,
"name": "PROB",
"pretty_name": null,
"description": "Probability that redshift is correct",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.085736Z",
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"unit": "-"
},
{
"id": 206,
"name": "RA",
"pretty_name": null,
"description": "RA of spectrum (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.111192Z",
"updated": "2021-02-09T04:07:37.793351Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 207,
"name": "SPECID",
"pretty_name": null,
"description": "Unique ID of spectrum",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.145700Z",
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"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 208,
"name": "SURVEY",
"pretty_name": null,
"description": "Survey this spectrum originated from",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.172922Z",
"updated": "2021-02-09T04:07:37.817699Z",
"contact": null,
"ucd": "meta.dataset",
"unit": "-"
},
{
"id": 209,
"name": "URL",
"pretty_name": null,
"description": "URL of the spectrum",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.200277Z",
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"unit": "-"
},
{
"id": 210,
"name": "URL_IMG",
"pretty_name": null,
"description": "URL of the spectrum`s image",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.219626Z",
"updated": "2021-02-09T04:07:37.841457Z",
"contact": null,
"ucd": "meta.ref.url;meta.file",
"unit": "-"
},
{
"id": 211,
"name": "WMAX",
"pretty_name": null,
"description": "Maximum wavelength of spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.243386Z",
"updated": "2021-02-09T04:07:37.864217Z",
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"ucd": "em.wl;stat.max",
"unit": "A"
},
{
"id": 212,
"name": "WMIN",
"pretty_name": null,
"description": "Minimum wavelength of spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.267847Z",
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},
{
"id": 213,
"name": "Z",
"pretty_name": null,
"description": "Heliocentric redshift",
"documentation": "",
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.297071Z",
"updated": "2021-02-09T04:07:37.887231Z",
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}
]
},
{
"id": 7,
"name": "ExternalSpecAll",
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"description": "This table lists all spectra of GAMA DR2 objects that are available from previous spectroscopic surveys (such as the SDSS), including duplicate observations. Every spectrum listed in this table is available in the GAMA DR2 database.",
"documentation": "",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/ExternalSpecAll.fits",
"file_name": "ExternalSpecAll.fits",
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"version": "v01",
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"created": "2021-01-28T00:39:53.416221Z",
"updated": "2021-02-09T04:07:34.662124Z",
"contact": {
"email": "jliske@eso.org",
"name": "Joe Liske "
},
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"columns": [
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"id": 226,
"name": "URL",
"pretty_name": null,
"description": "URL of the spectrum",
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.726328Z",
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},
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"description": "ID of matched GAMA object",
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.323705Z",
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},
{
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"description": "DEC of spectrum (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.366481Z",
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},
{
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"description": "Distance between spectrum and matched GAMA object",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.400506Z",
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},
{
"id": 217,
"name": "FILENAME",
"pretty_name": null,
"description": "Full path and filename of the spectrum",
"documentation": "",
"file_path": null,
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"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.428123Z",
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},
{
"id": 218,
"name": "GAMA_NAME",
"pretty_name": null,
"description": "Name of matched GAMA object",
"documentation": "",
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"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.446323Z",
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},
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"id": 219,
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"pretty_name": null,
"description": "Catalogue source(s) of matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.481281Z",
"updated": "2021-02-09T04:07:37.968101Z",
"contact": null,
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"unit": "-"
},
{
"id": 220,
"name": "IS_SBEST",
"pretty_name": null,
"description": "Is this the spectrum with the best redshift of this GAMA object within the originating survey?",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.512746Z",
"updated": "2021-02-09T04:07:37.988199Z",
"contact": null,
"ucd": "meta.code",
"unit": "-"
},
{
"id": 221,
"name": "NQ",
"pretty_name": null,
"description": "Normalised redshift quality (use nQ > 2 for science)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.541268Z",
"updated": "2021-02-09T04:07:37.999595Z",
"contact": null,
"ucd": "meta.code.qual;src.redshift",
"unit": "-"
},
{
"id": 222,
"name": "PROB",
"pretty_name": null,
"description": "Probability that redshift is correct",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.584616Z",
"updated": "2021-02-09T04:07:38.011044Z",
"contact": null,
"ucd": "stat.probability;src.redshift",
"unit": "-"
},
{
"id": 223,
"name": "RA",
"pretty_name": null,
"description": "RA of spectrum (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.627692Z",
"updated": "2021-02-09T04:07:38.031047Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 224,
"name": "SPECID",
"pretty_name": null,
"description": "Unique ID of spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.655217Z",
"updated": "2021-02-09T04:07:38.042589Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 225,
"name": "SURVEY",
"pretty_name": null,
"description": "Survey this spectrum originated from",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.690337Z",
"updated": "2021-02-09T04:07:38.053397Z",
"contact": null,
"ucd": "meta.dataset",
"unit": "-"
},
{
"id": 227,
"name": "URL_IMG",
"pretty_name": null,
"description": "URL of the spectrum`s image",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.754341Z",
"updated": "2021-02-09T04:07:38.084378Z",
"contact": null,
"ucd": "meta.ref.url;meta.file",
"unit": "-"
},
{
"id": 228,
"name": "WMAX",
"pretty_name": null,
"description": "Maximum wavelength of spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.772290Z",
"updated": "2021-02-09T04:07:38.096386Z",
"contact": null,
"ucd": "em.wl;stat.max",
"unit": "A"
},
{
"id": 229,
"name": "WMIN",
"pretty_name": null,
"description": "Minimum wavelength of spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.790305Z",
"updated": "2021-02-09T04:07:38.116415Z",
"contact": null,
"ucd": "em.wl;stat.min",
"unit": "A"
},
{
"id": 230,
"name": "Z",
"pretty_name": null,
"description": "Heliocentric redshift",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.817142Z",
"updated": "2021-02-09T04:07:38.127945Z",
"contact": null,
"ucd": "src.redshift",
"unit": "-"
}
]
},
{
"id": 8,
"name": "ExternalzAll",
"pretty_name": null,
"description": "This table lists a few redshifts of GAMA DR2 objects taken from the literature. The spectra from which these redshifts were measured are NOT available in the GAMA DR2 database.",
"documentation": "",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/ExternalzAll.fits",
"file_name": "ExternalzAll.fits",
"file_extension": "fits",
"version": "v01",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.440093Z",
"updated": "2021-02-09T04:07:34.681663Z",
"contact": {
"email": "jliske@eso.org",
"name": "Joe Liske "
},
"input_cat": false,
"columns": [
{
"id": 231,
"name": "CATAID",
"pretty_name": null,
"description": "ID of matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.872016Z",
"updated": "2021-02-09T04:07:38.139516Z",
"contact": null,
"ucd": "meta.id.cross;src",
"unit": "-"
},
{
"id": 232,
"name": "DEC",
"pretty_name": null,
"description": "DEC of spectrum (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.915018Z",
"updated": "2021-02-09T04:07:38.160245Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 233,
"name": "DIST",
"pretty_name": null,
"description": "Distance between spectrum and matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.942456Z",
"updated": "2021-02-09T04:07:38.172157Z",
"contact": null,
"ucd": "pos.angDistance",
"unit": "arcsec"
},
{
"id": 234,
"name": "GAMA_NAME",
"pretty_name": null,
"description": "Name of matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:00.969068Z",
"updated": "2021-02-09T04:07:38.184402Z",
"contact": null,
"ucd": "meta.id.cross;src",
"unit": "-"
},
{
"id": 235,
"name": "IC_FLAG",
"pretty_name": null,
"description": "Catalogue source(s) of matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.012338Z",
"updated": "2021-02-09T04:07:38.197519Z",
"contact": null,
"ucd": "meta.code.member",
"unit": "-"
},
{
"id": 236,
"name": "NQ",
"pretty_name": null,
"description": "Normalised redshift quality (use nQ > 2 for science)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.056587Z",
"updated": "2021-02-09T04:07:38.209621Z",
"contact": null,
"ucd": "meta.code.qual;src.redshift",
"unit": "-"
},
{
"id": 237,
"name": "PROB",
"pretty_name": null,
"description": "Probability that redshift is correct",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.100023Z",
"updated": "2021-02-09T04:07:38.223288Z",
"contact": null,
"ucd": "stat.probability;src.redshift",
"unit": "-"
},
{
"id": 238,
"name": "RA",
"pretty_name": null,
"description": "RA of spectrum (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.177011Z",
"updated": "2021-02-09T04:07:38.235020Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 239,
"name": "SPECID",
"pretty_name": null,
"description": "Unique ID of spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.220274Z",
"updated": "2021-02-09T04:07:38.247862Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 240,
"name": "SURVEY",
"pretty_name": null,
"description": "Survey this spectrum originated from",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.263120Z",
"updated": "2021-02-09T04:07:38.259634Z",
"contact": null,
"ucd": "meta.dataset",
"unit": "-"
},
{
"id": 241,
"name": "Z",
"pretty_name": null,
"description": "Heliocentric redshift",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.306111Z",
"updated": "2021-02-09T04:07:38.271701Z",
"contact": null,
"ucd": "src.redshift",
"unit": "-"
}
]
}
]
},
{
"id": 7,
"name": "GalexPhotometry",
"pretty_name": "GalexPhotometry",
"description": "This DMU provides GALEX NUV and FUV photometry for GAMA DR2 objects.",
"documentation": "GalexPhotometry<br>2012-11-13<br>Ellen Andrae <ellen.andrae@mpi-hd.mpg.de><br><br>This DMU provides GALEX NUV and FUV photometry for GAMA DR2 objects.<br><br>The GALEX ultraviolet data are a combination of archival data and<br>pointed observations from the GALEX guest investigator (GI) program<br>GALEX-GAMA: UV/Optical/Near-IR/Far-IR/Radio observations of ~100k<br>galaxies (GI5-048; PIs: R. Tuffs, C. Popescu, US-PI: M. Seibert). The<br>archival data have been used to extend the ultraviolet coverage of the<br>GAMA regions as much as possible.<br><br>The website of the GALEX-GAMA project is<br><a href=\"http://www.mpi-hd.mpg.de/galex-gama/\">www.mpi-hd.mpg.de/galex-gama/</a>.<br><br>This DMU provides several tables:<br><br>- GalexPhot<br> GALEX NUV and FUV photometry in the GAMA I survey regions provided<br> by the GALEX SExtractor-based pipeline.<br><br>- GalexObsInfo<br> Basic GALEX observational info for all GAMA DR2 objects, including<br> detection limits for the GALEX SExtractor-based pipeline.<br><br>- GalexSimpleMatch<br> Result for GAMA DR2 objects of a simple nearest neighbour match<br> between GalexPhot and InputCatA (within 4 arcsec).<br><br>- GalexAdvancedMatch<br> Result for GAMA DR2 objects of an advanced match between GalexPhot<br> and InputCatA. The advanced matching procedure attempts to<br> reconstruct the true UV flux of a given GAMA object in cases where<br> multiple GAMA and GALEX objects are associated with each other.<br><br>- GalexCoGPhot<br> GALEX NUV and FUV curve-of-growth photometry at the optical<br> positions of all GAMA DR2 objects.<br><br>- GalexMain<br> This is the main catalogue of this DMU. It should cover the needs of<br> most users. It duplicates the most important information from the<br> other catalogues in this DMU, and provides estimates of the \"best\"<br> NUV and FUV fluxes for all GAMA DR2 objects that were detected by<br> GALEX.<br><br><br>Dependencies<br>============<br>This DMU used the following inputs:<br><br> External GALEX pipeline v7<br> InputCat InputCatA v05<br> SersicPhotometry SersicCat v07<br><br><br>GALEX data<br>==========<br>All GI and archival data overlapping the GAMA I survey regions and<br>available as of 30 March 2010 were compiled for this project,<br>resulting in 212 GALEX tiles (circular fields 1 degree wide). These<br>data cover between 70% and 95% of the three equatorial regions.<br><br><br>Unique area (Primary vs Secondary)<br>==================================<br>GALEX tiles overlap one another. This, of course, is inevitable when<br>trying to cover a contiguous area with circular fields of view.<br>Furthermore, because we include archival survey data which is observed<br>on a sky grid system and pointed observations (which are not on the<br>sky grid system) the overlap is often very hap-hazard. There are<br>several ways to handle this such that we include only unique<br>detections and allow a precise footprint computation. We use a method<br>that optimizes the areal coverage and weights tiles with FUV coverage<br>highest.<br><br>For each GAMA region the GALEX tiles are rank-sorted by FUV exposure<br>time and secondary rank-sorted by NUV exposure time. This ensures that<br>any tile with FUV coverage takes precedence over any tile with only<br>NUV coverage (note that the FUV detector on GALEX is non-operational<br>at this time).<br><br>Once sorted, the footprint of each tile is derived from the relative<br>response map (effective exposure time map) by comparing it to all<br>neighboring tiles with a higher rank-order. In this way a \"primary<br>map\" is made for each tile indicating which parts of the field of view<br>are to be considered \"primary\" and which parts are to be considered<br>\"secondary\".<br><br>In this DMU we only consider the primary areas.<br><br>Note that photometric data from the secondary areas as provided by the<br>GALEX SExtractor-based pipeline are available at the GALEX-GAMA<br>website.<br><br><br>Photometry<br>==========<br>None of the fluxes and magnitudes presented in this DMU have been<br>corrected for the effect of foreground Milky Way dust extinction.<br>Should these corrections be required, they can be obtained from the<br>table <a href=\"/dr2/schema/table.php?name=GalacticExtinction\">GalacticExtinction</a> in the <a href=\"/dr2/schema/dmu.php?name=InputCat\">InputCat DMU</a>. <br><br>All photometry is on the AB system.<br><br>The photomtery produced by the GALEX SExtractor-based pipeline is<br>accompanied by artifact warning flags. We have *not* excluded any<br>objects from any tables in this DMU based on these flags. However, we<br>strongly recommend to select against objects that have the DICHROIC<br>REFLECTION or WINDOW REFLECTION flags raised as these reflections to<br>could lead to seriously corrupted fluxes (see the notes of the<br>GalexPhot table for details).<br><br>",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v02",
"type": "CatalogueGroup",
"created": "2021-01-28T00:39:52.941727Z",
"updated": "2021-02-09T04:07:34.450310Z",
"contact": {
"email": "ellen.andrae@mpi-hd.mpg.de",
"name": "Ellen Andrae "
},
"tables": [
{
"id": 9,
"name": "GalexAdvancedMatch",
"pretty_name": null,
"description": "This catalogue contains the result of an advanced match between InputCatA and GalexPhot, listing only objects included in DR2. The matching procedure takes into account the possibility of multiple matches between GALEX and GAMA objects and seeks to reconstruct the original UV flux of a given GAMA object. GAMA DR2 objects without a GALEX match are not included in this catalogue.",
"documentation": "GalexPhotometry<br>GalexAdvancedMatch<br>v02<br>2012-11-13<br>Ellen Andrae <ellen.andrae@mpi-hd.mpg.de><br><br>This catalogue contains the result of an advanced matching procedure<br>between InputCatA (GAMA's SDSS-based input catalogue^*) and GalexPhot.<br>The matching procedure takes into account the possibility of multiple<br>matches between GALEX and GAMA objects and seeks to reconstruct the<br>original UV flux of a given GAMA object.<br><br>This catalogue only includes matched GAMA DR2 objects with <br>S/N_NUV >= 2.5 in the redistributed flux FLUXSPLIT_NUV (see below).<br><br>Unmatched GAMA DR2 objects are not included in this catalogue. Refer to<br>the table GalexObsInfo for detection limits and to distinguish between<br>GAMA objects that were not detected in the GALEX data and those that<br>were not covered by GALEX.<br><br><br>Description of advanced matching procedure<br>==========================================<br>The advanced matching procedure takes into account the possibility of<br>multiple matches between GALEX and GAMA objects and seeks to<br>reconstruct the true UV flux of a given GAMA object.<br><br>We illustrate the routine for an example GAMA object. First, optical<br>shape information for the object (r-band ellipticity, position angle,<br>and effective radius) is extracted from the catalogue SersicCat,<br>and used to define a target area within which GALEX counterparts will<br>be deemed to be associated with the GAMA object. To take into account<br>scatter in apparent positions from real positions in the UV and<br>possibly unavailable optical shape information, the minimal search<br>region, i.e. optical target area, is a circle of radius 4 arcsec (the<br>matching radius used in GalexSimpleMatch). The question that is then<br>to be answered is which GALEX objects in GalexPhot have their central<br>coordinates within this optically defined search region. The number,<br>the IDs and the total flux of all such GALEX objects are recorded in<br>columns NMATCHUV, UVIDXLIST and FLUXTOT_XXX, respectively.<br><br>Since it is possible that a GALEX object may itself be extended, or<br>that it has more than one potential close-lying optical counterpart in<br>InputCatA, we also need to take into account the possibility that one<br>or more of the GALEX objects in the search region around the GAMA<br>object may themselves be related to further GAMA objects. Hence, in<br>the second step of the advanced matching procedure, a UV area is<br>constructed for each GALEX object within the optical search region,<br>using the object's position angle, ellipticity and size along its<br>semimajor axis from GalexPhot. InputCatA is then searched for GAMA<br>objects within the UV area of each of the GALEX objects. The number<br>and IDs of the GAMA objects found in this step are recorded in the<br>columns NMATCHOPT and OPTIDXLIST^*. The columns NMATCHUV and UVIDXLIST<br>for the GAMA objects found in this step are updated to include this<br>GALEX object.<br><br>In cases where there is a 1-to-1 match all of the flux of the GALEX<br>object is attributed to the matching GAMA object. This is by far the<br>most common case (68%). If, however, there is more than one potential<br>optical counterpart to one or more of the GALEX objects in the optical<br>search region, the UV flux of each of the GALEX objects is split among<br>all potential optical counterparts of that GALEX object, weighted<br>inversely by angular distance (using a minimum distance of 0.3 arcsec<br>to account for positional errors). Finally, the UV flux contributions<br>from all of the GALEX objects in the optical search radius to the GAMA<br>object under consideration are summed up and recorded in the columns<br>FLUXSPLIT_XXX. FLUXSPLITERR_XXX is the square-root of the weighted<br>quadratic sum of the errors of all GALEX objects from which the object<br>under consideration received a flux contribution, where the weights in<br>the quadratic sum are the same weights as those used for the flux<br>itself.<br><br>Finally, we purge from the catalogue all GAMA objects with<br>FLUXSPLIT_NUV / FLUXSPLITERR_NUV < 2.5.<br><br>Note that in cases where there is a 1-to-1 match between a GAMA and a<br>GALEX object we have FLUXTOT_XXX = FLUXSPLIT_XXX. Furthermore, in<br>these cases FLUXTOT_XXX is equal to FLUX_XXX from GalexPhot of the<br>GALEX object identified as the GAMA object's nearest GALEX neighbour<br>in GalexSimpleMatch. In other words, in these \"simple\" cases the<br>advanced matching procedure returns the same result for the UV fluxes<br>of a given GAMA object as the simple nearest neighbour matching.<br><br>Also note that it is possible for a GAMA object not to have a<br>FLUXTOT_XXX value associated with it but to still have a FLUXSPLIT_XXX<br>value associated with it. This will happen if there are no GALEX<br>objects within the GAMA object's optical search region (leading to<br>FLUXTOT_XXX being set to its default value of -99.0) and if the GAMA<br>object lies inside the UV search region(s) of one or more GALEX<br>objects, which in turn lie in the optical search region of at least<br>one other GAMA object. In this case the first GAMA object participates<br>in the re-distribution of the UV flux from these GALEX objects,<br>leading to FLUXSPLIT_XXX values != -99.0.<br><br>We also point out that there are substantial differences between the<br>objects included in this catalogue and those included in<br>GalexSimpleMatch. An object may be included in this catalogue but not<br>in GalexSimpleMatch and vice versa. The former happens when a GAMA<br>object is more than 4 arcsec away from its nearest GALEX neighbour but<br>still receives flux from one or more GALEX objects during the flux<br>re-distribution (with S/N_NUV >= 2.5). The latter happens when the<br>flux redistribution results in the S/N of the NUV flux received by a<br>GAMA object listed in GalexSimpleMatch dropping below the threshold of<br>2.5.<br><br>We recognise that the above flux redistribution scheme may not be<br>optimal, and that users may wish to apply other recipes for<br>distributing the UV flux among the optical counterparts (e.g. using<br>additional prior astrophysical information). This is easily achieved<br>given that we identify all GALEX and GAMA objects involved in a given<br>match in the columns UVIDXLIST and OPTIDXLIST^*.<br><br>We caution that the UV flux estimates reported in columns<br>FLUXSPLIT_XXX are only correct in a statistical sense, i.e. when<br>considering a large population of objects. However, for individual<br>objects they are necessarily imprecise.<br><br>The default value for non-measurements is -99.0.<br><br><br>^* Additional note<br>==================<br>This catalogue is actually slightly inconsistent with the rest of the<br>GAMA DR2 because the advanced matching procedure described above was<br>carried out using v06 of InputCatA, whereas the version released in<br>DR2 is <a href=\"/dr2/schema/table.php?name=InputCatA\">v05</a>. InputCatAv05 is the GAMA I master input catalogue, whereas<br>InputCatAv06 is the version used for GAMA II. v06 was chosen for the<br>advanced matching between GalexPhot and InputCatA because it has a<br>slightly fainter flux limit than v05 (r < 20.0 in v06 vs. r < 19.8 in<br>v05), and because it includes point sources (which were excluded from<br>v05). Both of these differences should make the matching and flux<br>re-distribution more reliable.<br><br>As explained above, column OPTIDXLIST lists all GAMA objects (using<br>the SDSS identifier OBJID) that are involved in the matching. However,<br>since InputCatAv06 contains significantly more objects than v05, a<br>number of the objects listed in column OPTIDXLIST are not found in<br>InputCatAv05 as released in GAMA DR2. To be precise, of the 62,036<br>unique objects listed in column OPTIDXLIST 9686 are not in<br>InputCatAv05. <br><br>Furthermore, we note that InputCatAv05 is based on SDSS DR6, whereas<br>InputCatAv06 is based on SDSS DR7. The SDSS OBJID used in column<br>OPTIDXLIST is hence the SDSS DR7 OBJID. However, since a small<br>fraction of objects changed their SDSS OBJID between DR6 and DR7,<br>there are 546 objects that are listed in column OPTIDXLIST with a<br>different OBJID than that used in InputCatAv05.<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/GalexAdvancedMatch.fits",
"file_name": "GalexAdvancedMatch.fits",
"file_extension": "fits",
"version": "v02",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.473372Z",
"updated": "2021-02-09T04:07:34.710537Z",
"contact": {
"email": "ellen.andrae@mpi-hd.mpg.de",
"name": "Ellen Andrae "
},
"input_cat": false,
"columns": [
{
"id": 263,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS objid",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.980063Z",
"updated": "2021-02-09T04:07:38.577341Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 242,
"name": "CATAID",
"pretty_name": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.350749Z",
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"contact": null,
"ucd": "meta.id",
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},
{
"id": 243,
"name": "FLUXSPLITERR_FUV",
"pretty_name": null,
"description": "Redistributed FUV flux error",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.384730Z",
"updated": "2021-02-09T04:07:38.297208Z",
"contact": null,
"ucd": "phot.flux;em.UV.100-200nm;stat.error",
"unit": "microJy"
},
{
"id": 244,
"name": "FLUXSPLITERR_NUV",
"pretty_name": null,
"description": "Redistributed NUV flux error",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.417948Z",
"updated": "2021-02-09T04:07:38.309541Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm;stat.error",
"unit": "microJy"
},
{
"id": 245,
"name": "FLUXSPLIT_FUV",
"pretty_name": null,
"description": "Redistributed FUV flux of all GALEX objects associated with GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.443401Z",
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"contact": null,
"ucd": "phot.flux;em.UV.100-200nm",
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},
{
"id": 246,
"name": "FLUXSPLIT_NUV",
"pretty_name": null,
"description": "Redistributed NUV flux of all GALEX objects associated with GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.469719Z",
"updated": "2021-02-09T04:07:38.336630Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm",
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},
{
"id": 247,
"name": "FLUXTOTERR_FUV",
"pretty_name": null,
"description": "Total FUV flux error",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.495887Z",
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},
{
"id": 248,
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"pretty_name": null,
"description": "Total NUV flux error",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.513580Z",
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"contact": null,
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"unit": "microJy"
},
{
"id": 249,
"name": "FLUXTOT_FUV",
"pretty_name": null,
"description": "Total FUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.555624Z",
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},
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"id": 250,
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"description": "Total NUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
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},
{
"id": 251,
"name": "FUVFLAG",
"pretty_name": null,
"description": "Combination of the FUV artifact flags of all GALEX objects involved in the matching",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.600614Z",
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},
{
"id": 252,
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"description": "Redistributed FUV AB magnitude error",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.625783Z",
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},
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"description": "Redistributed NUV AB magnitude error",
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},
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"description": "Redistributed FUV AB magnitude of all GALEX objects associated with GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.707411Z",
"updated": "2021-02-09T04:07:38.454955Z",
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"unit": "mag"
},
{
"id": 255,
"name": "MAGSPLIT_NUV",
"pretty_name": null,
"description": "Redistributed NUV AB magnitude of all GALEX objects associated with GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.735881Z",
"updated": "2021-02-09T04:07:38.475899Z",
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},
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"id": 256,
"name": "MAGTOTERR_FUV",
"pretty_name": null,
"description": "Total FUV AB magnitude error",
"documentation": "",
"file_path": null,
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"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.763511Z",
"updated": "2021-02-09T04:07:38.495604Z",
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"ucd": "phot.mag;em.UV.100-200nm;stat.error",
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},
{
"id": 257,
"name": "MAGTOTERR_NUV",
"pretty_name": null,
"description": "Total NUV AB magnitude error",
"documentation": "",
"file_path": null,
"file_name": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.798182Z",
"updated": "2021-02-09T04:07:38.507389Z",
"contact": null,
"ucd": "phot.mag;em.UV.200-300nm;stat.error",
"unit": "mag"
},
{
"id": 258,
"name": "MAGTOT_FUV",
"pretty_name": null,
"description": "Total FUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.833358Z",
"updated": "2021-02-09T04:07:38.518507Z",
"contact": null,
"ucd": "phot.mag;em.UV.100-200nm",
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},
{
"id": 259,
"name": "MAGTOT_NUV",
"pretty_name": null,
"description": "Total NUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.869767Z",
"updated": "2021-02-09T04:07:38.530582Z",
"contact": null,
"ucd": "phot.mag;em.UV.200-300nm",
"unit": "mag"
},
{
"id": 260,
"name": "NMATCHOPT",
"pretty_name": null,
"description": "Number of GAMA objects involved in the matching",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.913160Z",
"updated": "2021-02-09T04:07:38.542205Z",
"contact": null,
"ucd": "meta.number",
"unit": "-"
},
{
"id": 261,
"name": "NMATCHUV",
"pretty_name": null,
"description": "Number of GALEX objects involved in the matching",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.931631Z",
"updated": "2021-02-09T04:07:38.553806Z",
"contact": null,
"ucd": "meta.number",
"unit": "-"
},
{
"id": 262,
"name": "NUVFLAG",
"pretty_name": null,
"description": "Combination of the NUV artifact flags of all GALEX objects involved in the matching",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.959500Z",
"updated": "2021-02-09T04:07:38.565722Z",
"contact": null,
"ucd": "meta.code;em.UV.200-300nm",
"unit": "-"
},
{
"id": 264,
"name": "OPTIDXLIST",
"pretty_name": null,
"description": "ID list of GAMA objects used in the flux redistribution calculation using SDSS OBJID; string always ends with a comma",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:01.999880Z",
"updated": "2021-02-09T04:07:38.588935Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 265,
"name": "UVIDXLIST",
"pretty_name": null,
"description": "ID list of GALEX object used in the flux redistribution calculation using NAME from GalexPhot; string always ends with a comma",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.019121Z",
"updated": "2021-02-09T04:07:38.600180Z",
"contact": null,
"ucd": "-",
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}
]
},
{
"id": 10,
"name": "GalexCoGPhot",
"pretty_name": null,
"description": "This catalogue provides GALEX NUV and FUV curve-of-growth photometry for all GAMA DR2 objects.",
"documentation": "GalexPhotometry<br>GalexCoGPhot<br>v02<br>2012-11-13<br>Ellen Andrae <ellen.andrae@mpi-hd.mpg.de><br><br>In addition to the GALEX-pipeline-generated photometry of \"blind\"<br>GALEX NUV detections presented in GalexPhot, we provide in this<br>catalogue NUV and FUV photometric measurements at the a priori known<br>optical positions of GAMA DR2 objects using a curve-of-growth (CoG)<br>method.<br><br>Our CoG method (described in detail below) requires not only the<br>positions but also the ellipticities and position angles of the<br>galaxies to be photometered. We take this information from the most<br>reliable source of shape information for GAMA galaxies, <a href=\"/dr2/schema/table.php?name=SersicCatAll\">SersicCatAll</a><br>in the <a href=\"/dr2/schema/dmu.php?name=SersicPhotometry\">SersicPhotometry DMU</a>.<br><br><br>Description of CoG method<br>=========================<br>For each object to be analysed, the local background level and its<br>(Poissonian) error, sigma_bkg, is estimated in the NUV/FUV data at the<br>object's optical position, and the background is subtracted. An<br>elliptical aperture is constructed from the object's r-band position,<br>effective radius (GAL_RE_R), ellipticity (GAL_ELLIP_R) and position<br>angle (GAL_PA_R) from SersicCatAll. This aperture is then convolved<br>with the GALEX PSF, assumed to be a Gaussian with a FWHM of 5.3 arcsec.<br><br>The flux is then averaged in elliptical annuli of the above shape of<br>width 3 arcsec (as measured along the object's major axis). The<br>\"integration radius\" (along the major axis) of the target is then<br>defined as the smaller of the following: the outer radius of the<br>smallest annulus in which the average flux falls below the background<br>level plus 1.0 sigma_bkg or the outer radius + 3 arcsec of the<br>smallest annulus in which the average flux falls below the background<br>level plus 1.5 sigma_bkg. This was found to be a good compromise<br>between including very faint target emission at large radii on the one<br>hand and the need to avoid pure noise integration or blending with<br>neighbouring objects on the other. This integration radius is listed<br>in columns RE_CRIT_XXX in the catalogue.<br><br>Objects for which the flux in the innermost annulus (0-3 arcsec) is<br>already below the level of the background plus 1.5 sigma_bkg have<br>RE_CRIT_XXX set to 0. Furthermore, objects with RE_CRIT_XXX = 3 arcsec<br>must also be considered non-detections since they are smaller than the<br>GALEX PSF.<br><br>The flux of the target is then determined by integrating the flux<br>inside the elliptical aperture of size RE_CRIT_XXX. If this flux is<br>negative (i.e. a complete non-detection) then all flux columns are set<br>to 99. Note that apart from this \"cut\", all flux measurements are<br>reported in this catalogue, i.e. no S/N limit is applied.<br><br>In order to avoid contamination from neighbouring sources (taken from<br>InputCatA), a circular area with a radius (not diameter) of 5.3 arcsec<br>is masked around these. Any masked pixels inside a galaxy's<br>integration aperture are accounted for by renormalizing the unmasked<br>galaxy flux measured in the same elliptical annuli as the masked<br>pixels. Galaxies where this was necessary are flagged in the columns<br>CONFSOURCE_XXX. Objects for which the flux profile never reaches the<br>level of the background plus 1.5 sigma_bkg due to the flux of<br>neighbouring objects outside of their masks have their fluxes set to<br>999. Objects with a masked area in the central radius bin are deemed<br>to be unmeasurable and their flux values are set to -99.<br><br>Objects with RE_CRIT_NUV > RE_CRIT_FUV + 30 arcsec are very likely to<br>have a NUV measurement that was contaminated by a neighboring<br>source. (Especially stars tend to be much fainter in the FUV, thus<br>even very bright stars are very unlikely to have excess FUV flux<br>outside the masked area, even though they may have excess NUV flux<br>outside the masked area.) Therefore, all NUV columns are set to 999 in<br>these cases.<br><br>Objects not covered by the GALEX data (or those where the coverage of<br>the surroundings was not sufficient for a background estimate) also<br>have their fluxes set to -99.<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/GalexCoGPhot.fits",
"file_name": "GalexCoGPhot.fits",
"file_extension": "fits",
"version": "v02",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.492725Z",
"updated": "2021-02-09T04:07:34.744893Z",
"contact": {
"email": "ellen.andrae@mpi-hd.mpg.de",
"name": "Ellen Andrae "
},
"input_cat": false,
"columns": [
{
"id": 278,
"name": "HP_RAD_NUV",
"pretty_name": null,
"description": "NUV radius enclosing 50% of the total flux",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.477241Z",
"updated": "2021-02-09T04:07:38.789603Z",
"contact": null,
"ucd": "phys.size.radius;em.UV.200-300nm",
"unit": "arcsec"
},
{
"id": 283,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS objid",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.585852Z",
"updated": "2021-02-09T04:07:38.852661Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 266,
"name": "CATAID",
"pretty_name": null,
"description": "Unique ID of GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.062530Z",
"updated": "2021-02-09T04:07:38.611502Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 267,
"name": "CONFSOURCE_FUV",
"pretty_name": null,
"description": "FUV flag indicating whether masking occurred",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.105900Z",
"updated": "2021-02-09T04:07:38.623229Z",
"contact": null,
"ucd": "meta.code",
"unit": "-"
},
{
"id": 268,
"name": "CONFSOURCE_NUV",
"pretty_name": null,
"description": "NUV flag indicating whether masking occurred",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.141575Z",
"updated": "2021-02-09T04:07:38.634822Z",
"contact": null,
"ucd": "meta.code",
"unit": "-"
},
{
"id": 269,
"name": "CPSERR_FUV",
"pretty_name": null,
"description": "FUV counts per second error",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.196488Z",
"updated": "2021-02-09T04:07:38.646402Z",
"contact": null,
"ucd": "phot.count;em.UV.100-200nm;stat.error",
"unit": "counts/s"
},
{
"id": 270,
"name": "CPSERR_NUV",
"pretty_name": null,
"description": "NUV counts per second error",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.239114Z",
"updated": "2021-02-09T04:07:38.657631Z",
"contact": null,
"ucd": "phot.count;em.UV.200-300nm;stat.error",
"unit": "counts/s"
},
{
"id": 271,
"name": "CPS_FUV",
"pretty_name": null,
"description": "FUV counts per second",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.283068Z",
"updated": "2021-02-09T04:07:38.669090Z",
"contact": null,
"ucd": "phot.count;em.UV.100-200nm",
"unit": "counts/s"
},
{
"id": 272,
"name": "CPS_NUV",
"pretty_name": null,
"description": "NUV counts per second",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.326650Z",
"updated": "2021-02-09T04:07:38.680709Z",
"contact": null,
"ucd": "phot.count;em.UV.200-300nm",
"unit": "counts/s"
},
{
"id": 273,
"name": "FLUXERR_FUV",
"pretty_name": null,
"description": "FUV flux error",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.368907Z",
"updated": "2021-02-09T04:07:38.692420Z",
"contact": null,
"ucd": "phot.flux;em.UV.100-200nm;stat.error",
"unit": "microJy"
},
{
"id": 274,
"name": "FLUXERR_NUV",
"pretty_name": null,
"description": "NUV flux error",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.387758Z",
"updated": "2021-02-09T04:07:38.720143Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm;stat.error",
"unit": "microJy"
},
{
"id": 275,
"name": "FLUX_FUV",
"pretty_name": null,
"description": "FUV flux",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.408298Z",
"updated": "2021-02-09T04:07:38.741371Z",
"contact": null,
"ucd": "phot.flux;em.UV.100-200nm",
"unit": "microJy"
},
{
"id": 276,
"name": "FLUX_NUV",
"pretty_name": null,
"description": "NUV flux",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:02.428462Z",
"updated": "2021-02-09T04:07:38.763762Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm",
"unit": "microJy"
},
{
"id": 277,
"name": "HP_RAD_FUV",
"pretty_name": null,
"description": "FUV radius enclosing 50% of the total flux",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
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"id": 279,
"name": "MAGERR_FUV",
"pretty_name": null,
"description": "FUV magnitude error",
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"description": "NUV magnitude error",
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"name": "MAG_FUV",
"pretty_name": null,
"description": "FUV magnitude",
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"name": "MAG_NUV",
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"name": "RE_CRIT_FUV",
"pretty_name": null,
"description": "FUV integration radius (multiple of 3 arcsec)",
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"description": "NUV integration radius (multiple of 3 arcsec)",
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]
},
{
"id": 11,
"name": "GalexMain",
"pretty_name": null,
"description": "This is the main catalogue of the GalexPhotometry DMU. It reproduces the most important information from the other catalogues in this DMU and provides a best estimate of the NUV and FUV fluxes of all GAMA DR2 objects that were detected by GALEX.",
"documentation": "GalexPhotometry<br>GalexMain<br>v02<br>2012-11-13<br>Ellen Andrae <ellen.andrae@mpi-hd.mpg.de><br><br>This is the main catalogue of the GalexPhotometry DMU. It reproduces<br>the most important information from the other catalogues in this DMU<br>and provides a best estimate of the NUV and FUV fluxes of all GAMA DR2<br>objects that were detected by GALEX.<br><br>Included in this catalogue are all GAMA DR2 objects that either<br><br>- have an entry in GalexSimpleMatch<br>or<br>- have an entry in GalexAdvancedMatch<br>or<br>- have an entry in GalexCoGPhot with S/N_NUV >= 2.5 and integration<br> radius RE_CRIT_NUV >= 6 arcsec<br><br>The S/N criterion applied to GalexCoGPhot is the same as that used for<br>GalexPhot and GalexAdvancedMatch. Note that GAMA DR2 objects that were<br>not detected by GALEX (in the sense that they do not match any of the<br>criteria above) are not included in this catalogue. Refer to the table<br>GalexObsInfo for nominal detection limits and to distinguish between<br>GAMA objects that were not detected in the GALEX data and those that<br>were not covered by GALEX. For DR2 objects not included in the present<br>catalogue you can also turn to the table GalexCoGPhot to find out if<br>they were \"detected\" at S/N_NUV < 2.5, i.e. essentially to find upper<br>flux limits for these objects.<br><br>This catalogue provides the following information:<br><br>- In columns 50-75 (NN_GGOID - NN_POSANGERR_NUV) we reproduce the main<br> information on the GAMA object's nearest neighbour GALEX object from<br> GalexPhot (catalogue of UV detections and photometry from the GALEX<br> SExtractor-based pipeline), using GalexSimpleMatch to connect the<br> two. The columns NN_FLUX_XXX contain the fluxes of the nearest<br> neighbour GALEX object as measured by the GALEX SExtractor-based<br> pipeline. For more information refer to the notes of the<br> GalexSimpleMatch and GalexPhot tables.<br><br>- In columns 16-35 (NMATCHUV - SPLIT_MAGERR_FUV) we reproduce the main<br> information from GalexAdvancedMatch. This table contains the result<br> (for GAMA DR2 objects) of an advanced match between GalexPhot and<br> InputCatA. The advanced matching procedure attempts to reconstruct<br> the true UV flux of a given GAMA object in cases where multiple GAMA<br> and GALEX objects are associated with each other. This reconstructed<br> flux is reported in columns SPLIT_FLUX_XXX. The columns TOT_FLUX_XXX<br> contain the total flux of all GALEX objects associated with a given<br> GAMA object. For more information refer to the notes of the<br> GalexAdvancedMatch table.<br><br>- In columns 36-49 (COG_FLUX_NUV - COG_CONFSOURCE_FUV) we reproduce<br> the main information from GalexCoGPhot. This table contains<br> photometric measurements (using a curve-of-growth method) at the a<br> priori known optical positions of GAMA objects. The columns<br> COG_FLUX_XXX contain the fluxes returned by the CoG method. For more<br> information refer to the notes of the GalexCoGPhot table.<br><br>- In columns 7-15 (BEST_FLUX_NUV - BEST_METHOD) we report our best<br> estimate of the NUV and FUV fluxes of a given GAMA object. In these<br> columns we make appropriate choices among the various fluxes<br> available for a given object (from the advanced matching or CoG<br> methods), and we strongly recommend the use of these BEST fluxes.<br><br> In cases where there is an unambiguous 1-to-1 correspondence between<br> a GAMA and a GALEX object we believe the fluxes returned by the<br> GALEX pipeline for the GALEX object to be the most appropriate. Note<br> that in these cases the nearest neighbour and advanced matching<br> procedures of course return the same results for the UV fluxes of a<br> given GAMA object, i.e. NN_FLUX_XXX = TOT_FLUX_XXX = SPLIT_FLUX_XXX.<br> <br> In cases where the GAMA object is very extended or where there are<br> multiple GAMA and/or GALEX objects associated with each other we<br> believe our CoG photometry to be superior. <br><br> However, in cases where the CoG measurements have failed (for<br> whatever reason, see the notes of the GalexCoGPhot table) we resort<br> to the reconstructed fluxes SPLIT_FLUX_XXX returned by the advanced<br> matching procedure.<br><br> We therefore set BEST_FLUX_XXX according to the following rules: <br><br> - If only one of COG_FLUX_NUV and SPLIT_FLUX_NUV is available in<br> this catalogue then the BEST columns are set to the corresponding<br> columns of the available flux method.<br><br> - If both COG_FLUX_NUV and SPLIT_FLUX_NUV are available in this<br> catalogue then the BEST columns are set to the corresponding<br> columns of the CoG method if NMATCHUV > 1 or NMATCHOPT > 1 or<br> GAL_RE_R > 10 arcsec, where GAL_RE_R is the r-band effective<br> radius from SersicCatAll. Otherwise the BEST columns are set to<br> the corresponding SPLIT columns.<br><br> The flux method used for the BEST columns is recorded in column<br> BEST_METHOD (CoG or AdvancedMatch).<br><br> Note that for a COG_FLUX_NUV value to be present *in this catalogue*<br> it must have S/N >= 2.5 (see above).<br><br> Also note that there are 250 objects in this catalogue with neither<br> AdvancedMatch nor CoG entries. These objects were included here only<br> because they have an entry in GalexSimpleMatch, meaning they have at<br> least one S/N_NUV >= 2.5 GALEX object from GalexPhot within 4 arcsec. <br> However, all of these have multiple GALEX objects associated with<br> them. Hence one should not be tempted to use the UV flux of the<br> nearest GALEX neighbour as the BEST flux in these cases.<br><br><br>The default value for missing entries in this table is -999.<br><br>",
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"created": "2021-01-28T00:39:53.511506Z",
"updated": "2021-02-09T04:07:34.778118Z",
"contact": {
"email": "ellen.andrae@mpi-hd.mpg.de",
"name": "Ellen Andrae "
},
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"id": 328,
"name": "NN_MAGERR_NUV",
"pretty_name": null,
"description": "NUV AB Kron magnitude error of nearest neighbour GALEX object",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:03.656906Z",
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"contact": null,
"ucd": "phot.mag;em.UV.200-300nm;stat.error",
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"id": 343,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS objid",
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:03.986111Z",
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"name": "BEST_FLUXERR_FUV",
"pretty_name": null,
"description": "Best estimate FUV flux error",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:02.662156Z",
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"description": "Best estimate NUV flux error",
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"created": "2021-01-28T00:40:02.680534Z",
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"description": "Best estimate of the GAMA object`s FUV flux",
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"description": "Best estimate FUV magnitude error",
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"created": "2021-01-28T00:40:02.731370Z",
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"description": "Best estimate of the GAMA object`s FUV magnitude",
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"description": "Best estimate of the GAMA object`s NUV magnitude",
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"description": "Unique ID of GAMA object",
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"description": "CoG NUV integration radius (multiple of 3 arcsec)",
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{
"id": 310,
"name": "DEC",
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"description": "Declination of GAMA object (J2000)",
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"created": "2021-01-28T00:40:03.234024Z",
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"documentation": "GalexPhotometry<br>GalexPhot<br>v02<br>2012-11-13<br>Mark Seibert <mseibert@obs.carnegiescience.edu><br> <br>This catalogue provides GALEX NUV and FUV photometry for primary<br>sources with S/N_NUV >= 2.5 in the GAMA I survey regions. The present<br>catalogue was created at Caltech using a new version of the GALEX<br>SExtractor-based pipeline (v7).<br><br><br>Some points to note<br>===================<br>Matched apertures: This catalogue is NUV-centric. The S/N of the<br>NUV data is significantly higher than that of the FUV data. We have<br>taken advantage of this by performing source detection only in the<br>NUV, and then carrying out photometry in both bands in apertures<br>defined in the NUV. This has the advantage of improving the<br>reliability and completeness of the FUV detections and providing<br>meaningful UV colors. Please note however that, because source<br>detection is carried out in the NUV, it is possible to obtain negative<br>flux measurements in the FUV. Note also that all catalogue columns<br>without an explicit band reference are derived from the NUV.<br><br>Calibration: The major changes to the GALEX calibration compared to<br>previous versions include updates to the flat fields, flux response<br>trend with time, and a magnitude zero-point correction (0.043 mag<br>fainter in NUV and 0.033 mag fainter in FUV). Further information can<br>be found on the GALEX web page or detailed in <a href=\"http://www.galex.caltech.edu/researcher/gr6_docs/GI_Doc_Ops7.pdf\">this document</a>. Note that<br>due to the time trend and flat field changes one cannot simply apply<br>fixed zero-point corrections to the previus versions of this<br>catalogue.<br><br>Deblending/Shredding: The deblending threshold parameter has been<br>modified to improve the shredding of extended sources. Prior to v7 the<br>pipeline was tuned for point sources. With v7 a better compromise has<br>been reached that reduces the shredding for extended objects less than<br>1 arcmin in diameter.<br><br>Astrometry: The GALEX PSF is ~5 arcsec and the astrometry is only<br>accurate to within ~0.3 arcsec. Analysing the offsets between GALEX<br>and GAMA optical positions we find that the offsets are not systematic<br>and vary from GALEX tile to tile. The principle cause of the<br>astrometric offsets is the limited precision of astrometric catalogues<br>used to derive the plate solutions within the GALEX pipeline.<br><br>Finally we note that the present version of this catalogue was created<br>using the methods and techniques of the GALEX CATalog Team<br>(GCATT). This is a large project underway to produce a definitive<br>GALEX source catalogue.<br><br><br>Artifact flags<br>==============<br>This catalogue contains artifact warning flags for both the NUV and the<br>FUV. These are bitwise-encoded unsigned integers, each of which is the<br>bitwise logical 'or' of some or none of the possible flags listed<br>below. The flags are applied to regions of the image derived entirely<br>from geometry based on knowledge of the detector's orientation and<br>(for some flags) an a priori estimate of the NUV/FUV brightness of<br>known stars. Source brightness criteria for flagging are generous,<br>meaning that false-positives, especially for 'edge' flags, are common.<br>False-negatives are much rarer, but definitely occur with some<br>regularity.<br><br>In practice, the DICHROIC REFLECTION and WINDOW REFLECTION flags are<br>the only flags that one should always select against as these could<br>lead to seriously corrupt fluxes.<br><br><br>Flag name | Bit | Flag value | Meaning <br> | (LSB=1) | (base 10) | <br> ----------|---------|--------------------------------------------------------<br> Edge | 1 | 1 | Detector bevel edge reflection (NUV only) <br> ----------|---------|--------------------------------------------------------<br> Window | 2 | 2 | Detector window reflection (NUV only) <br> ----------|---------|--------------------------------------------------------<br> Dichroic | 3 | 4 | Dichroic reflection <br> ----------|---------|--------------------------------------------------------<br> Varpix | 4 | 8 | Varible pixel based on time slices.<br> ----------|---------|--------------------------------------------------------<br> Brtedge | 5 | 16 | Bright star near edge of field (NUV only).<br> | | | Just like #1 but with a higher count rate <br> | | | requirement (about 10 cps) on the <br> | | | generating star. Cuts down on false <br> | | | positives at the cost of a higher false <br> | | | negative rate. <br> ----------|---------|--------------------------------------------------------<br> Rim | 6 | 32 | Detector rim (annulus) proximity <br> | | | (>0.6 deg > from FOV center). <br> ----------|---------|--------------------------------------------------------<br> Dimask | 7 | 64 | Dichroic reflection artifact mask flag. <br> | | | Used only when a coadd has enough visits <br> | | | at enough position angles that masking <br> | | | the dichroic reflection doesn't decrease <br> | | | flux by more than 1/3. <br> ----------|---------|--------------------------------------------------------<br> Varmask | 8 | 128 | Masked pixel determined by varpix. <br> ----------|---------|--------------------------------------------------------<br> Hotmask | 9 | 256 | Masked detector hotspots.<br><br><br>As an example, if pixel N for an image is overlayed by an edge<br>reflection region and is in the rim region (i.e. near the detector<br>edge), its value is:<br><br>Flag(N) = 2^(1 - 1) = 1 (edge condition)<br><br>or 2^(6 - 1) = 32 (rim condition)<br><br>1 + 32 = 33 (bit coded value for both conditions)<br><br><br>Default values<br>==============<br>The default value for blank entries is -99 (used e.g. for FUV<br>quantities when FUV data are missing). The value 99 is assigned to<br>magnitudes when the corresponding flux is negative (see above).<br><br><br>Known issues<br>============<br>This catalogue contains a few GALEX objects which are closer to their<br>nearest GALEX neighbor than the FWHM of the GALEX PSF. These duplicate<br>detections are an artifact of the mosaicing of the primary areas: in<br>these cases an object is detected separately on two different tiles<br>with slightly different coordinates, and with each detection lying in<br>the primary area of its tile.<br><br>",
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"description": "This catalogue contains the result of a simple nearest neighbour match between InputCatA and GalexPhot, listing only objects included in DR2. GAMA DR2 objects without a GALEX nearest neighbour within a distance of 4 arcsec are considered unmatched and are not included in this catalogue.",
"documentation": "GalexPhotometry<br>GalexSimpleMatch<br>v02<br>2012-11-13<br>Ellen Andrae <ellen.andrae@mpi-hd.mpg.de><br><br>This catalogue contains the result of a simple nearest neighbour match<br>between InputCatA (the GAMA I SDSS-based input catalogue) and<br>GalexPhot. For each GAMA DR2 object this catalogue lists its nearest<br>neighbour GALEX object provided that the distance between the two is<br>less than 4 arcsec. GAMA DR2 objects without a GALEX nearest neighbour<br>within a distance of 4 arcsec are considered unmatched and are not<br>included in this catalogue. Refer to the table GalexObsInfo for<br>detection limits and to distinguish between GAMA objects that were not<br>detected in the GALEX data and those that were not covered by GALEX.<br><br>To obtain the properties of a given GAMA object's nearest neighbour<br>GALEX object simply join this table with the table GalexPhot on the<br>column GGOID.<br><br>Note that the resolution of the GALEX imaging is ~5 arcsec. This<br>obviously means that a given GALEX detection in GalexPhot may not<br>represent the UV flux of a single GAMA object (defined in the optical)<br>but the joint UV flux of multiple GAMA objects. In these cases it<br>would be incorrect to assign all of the GALEX flux to any single GAMA<br>object. Furthermore, doing so would introduce an environmental bias:<br>GAMA objects with many other close-by objects would be more likely to<br>be associated with a GALEX detection than isolated GAMA objects.<br><br>Hence, as a quality indicator of the match, the number of GALEX<br>objects within 4 arcsec distance to the GAMA objects is listed in<br>column NMATCH4. The column MANY2ONE gives the number of GAMA objects<br>this GALEX object has been matched to. If one of these two columns is<br>larger than 1, this must be considered a multiple match and we<br>recommend the use of the BEST_FLUX_XXX columns in GalexMain instead of<br>the nearest neighbour fluxes.<br><br>Further GALEX objects within a matching radius of 20 arcsec are also<br>listed (in columns GNEIGHBOR_*) to indicate potential multiple<br>matches.<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/GalexSimpleMatch.fits",
"file_name": "GalexSimpleMatch.fits",
"file_extension": "fits",
"version": "v02",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.601056Z",
"updated": "2021-02-09T04:07:34.816384Z",
"contact": {
"email": "ellen.andrae@mpi-hd.mpg.de",
"name": "Ellen Andrae "
},
"input_cat": false,
"columns": [
{
"id": 494,
"name": "CATAID",
"pretty_name": null,
"description": "Unique ID of GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.102511Z",
"updated": "2021-02-09T04:07:41.964667Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 495,
"name": "FUVMATCH",
"pretty_name": null,
"description": "Flag indicating whether matched GALEX source has FUV flux with S/N >=2.5 (-1=no FUV data)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.122841Z",
"updated": "2021-02-09T04:07:41.976934Z",
"contact": null,
"ucd": "meta.code;em.UV.100-200nm",
"unit": "-"
},
{
"id": 496,
"name": "GGOID",
"pretty_name": null,
"description": "Global Object ID of nearest neighbour GALEX object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.142220Z",
"updated": "2021-02-09T04:07:41.991045Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 497,
"name": "GNEIGHBOR_DIST",
"pretty_name": null,
"description": "String list of distances to all GALEX sources within 20 arcsec",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.161235Z",
"updated": "2021-02-09T04:07:42.004510Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 498,
"name": "GNEIGHBOR_NAME",
"pretty_name": null,
"description": "String list of names of all GALEX sources within 20 arcsec",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.231724Z",
"updated": "2021-02-09T04:07:42.053081Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 499,
"name": "MANY2ONE",
"pretty_name": null,
"description": "Number of GAMA objects the GALEX object is matched to",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.284730Z",
"updated": "2021-02-09T04:07:42.085234Z",
"contact": null,
"ucd": "meta.number",
"unit": "-"
},
{
"id": 500,
"name": "NMATCH4",
"pretty_name": null,
"description": "Number of GALEX objects found within 4 arcsec of GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.320791Z",
"updated": "2021-02-09T04:07:42.100520Z",
"contact": null,
"ucd": "meta.number",
"unit": "-"
},
{
"id": 501,
"name": "NN_DIST",
"pretty_name": null,
"description": "Distance between GAMA object and nearest neighbour GALEX object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.363637Z",
"updated": "2021-02-09T04:07:42.112890Z",
"contact": null,
"ucd": "pos.angDistance",
"unit": "arcsec"
},
{
"id": 502,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS objid of GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.384205Z",
"updated": "2021-02-09T04:07:42.126118Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
}
]
},
{
"id": 12,
"name": "GalexObsInfo",
"pretty_name": null,
"description": "This catalogue provides basic GALEX observational information, i.e. exposure times, background levels and detection limits, for all GAMA DR2 objects.",
"documentation": "GalexPhotometry<br>GalexObsInfo<br>v02<br>2012-11-13<br>Ellen Andrae <ellen.andrae@mpi-hd.mpg.de><br> <br>This catalogue provides basic GALEX observational information,<br>i.e. exposure times, background levels and GALEX Sextractor-based<br>pipeline detection limits, for (almost) all DR2 objects. (Eleven DR2<br>objects had to be excluded for technical reasons.)<br><br>This catalogue includes all objects that are currently not covered by<br>GALEX NUV data. The rows for these objects are \"empty\" (containing<br>-99). As the matched catalogues GalexSimpleMatch and<br>GalexAdvancedMatch only contain matched objects, we report these<br>\"empty\" rows here to enable the user to discriminate between objects<br>that were covered by GALEX (in the NUV) but not detected, and those<br>that were not covered by GALEX.<br><br><br>Detection limits<br>================<br>The columns NUVFLUXLIMITXX and FUVFLUXLIMITXX give the GALEX<br>Sextractor-based pipeline detection limits at this position for a<br>circular source for the given signal-to-noise cut. They use a default<br>radius of 3.4\" or, if it is listed and greater than 3.4\", the radius<br>given by GAL_RE_R in SersicCatv07. (Note that SersicCatv07 only covers<br>the nominal GAMA I survey regions, which are sub-regions of the<br>nominal GAMA II survey regions, which are in turn sub-regions of the<br>regions covered by InputCatAv06.)<br><br>Users can calculate detection limits in units of counts per second for<br>any desired signal-to-noise ration (SN) themselves using the formula:<br><br>fluxlimitcps = ((SN)^2 + sqrt((SN)^4 + 4*eff_exptime*limcat*area*(SN)^2)) / (2*eff_exptime)<br><br>where NUV or FUV quantities should be used accordingly. \"limcat\"<br>denotes the background brightness in counts per second, defined as<br>follows in terms of the columns BKGRND_FLUX_NUV and BKGRND_FLUX_FUV:<br><br>limcat = BKGRND_FLUX / CUJ<br><br>where CUJ_NUV = 33.7286987304688 and CUJ_FUV = 107.647003173828.<br><br>To obtain fluxlimits in microJy, use <br><br>fluxlimit = fluxlimitcps * CUJ<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/GalexObsInfo.fits",
"file_name": "GalexObsInfo.fits",
"file_extension": "fits",
"version": "v02",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.538567Z",
"updated": "2021-02-09T04:07:34.792378Z",
"contact": {
"email": "ellen.andrae@mpi-hd.mpg.de",
"name": "Ellen Andrae "
},
"input_cat": false,
"columns": [
{
"id": 371,
"name": "FUVMAGLIMIT5",
"pretty_name": null,
"description": "S/N=5 FUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.575258Z",
"updated": "2021-02-09T04:07:40.117653Z",
"contact": null,
"ucd": "phot.mag;em.UV.100-200nm;stat.min",
"unit": "mag"
},
{
"id": 361,
"name": "BKGRND_FLUX_FUV",
"pretty_name": null,
"description": "FUV sky background surface brightness",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.356079Z",
"updated": "2021-02-09T04:07:39.954069Z",
"contact": null,
"ucd": "phot.flux;em.UV.100-200nm;src.net",
"unit": "microJy/arcsec^2"
},
{
"id": 362,
"name": "BKGRND_FLUX_NUV",
"pretty_name": null,
"description": "NUV sky background surface brightness",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.379076Z",
"updated": "2021-02-09T04:07:39.966597Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm;src.net",
"unit": "microJy/arcsec^2"
},
{
"id": 363,
"name": "CATAID",
"pretty_name": null,
"description": "Unique ID of GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.397853Z",
"updated": "2021-02-09T04:07:39.988240Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 364,
"name": "EFF_EXPTIME_FUV",
"pretty_name": null,
"description": "FUV effective exposure time (relative response)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.415843Z",
"updated": "2021-02-09T04:07:40.001627Z",
"contact": null,
"ucd": "obs.exposure;em.UV.100-200nm",
"unit": "s"
},
{
"id": 365,
"name": "EFF_EXPTIME_NUV",
"pretty_name": null,
"description": "NUV effective exposure time (relative response)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.433620Z",
"updated": "2021-02-09T04:07:40.015726Z",
"contact": null,
"ucd": "obs.exposure;em.UV.200-300nm",
"unit": "s"
},
{
"id": 366,
"name": "FUVFLUXLIMIT10",
"pretty_name": null,
"description": "S/N=10 FUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.452595Z",
"updated": "2021-02-09T04:07:40.028858Z",
"contact": null,
"ucd": "phot.flux;em.UV.100-200nm;stat.min",
"unit": "microJy"
},
{
"id": 367,
"name": "FUVFLUXLIMIT2p5",
"pretty_name": null,
"description": "S/N=2.5 FUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.480064Z",
"updated": "2021-02-09T04:07:40.043491Z",
"contact": null,
"ucd": "phot.flux;em.UV.100-200nm;stat.min",
"unit": "microJy"
},
{
"id": 368,
"name": "FUVFLUXLIMIT5",
"pretty_name": null,
"description": "S/N=5 FUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.497034Z",
"updated": "2021-02-09T04:07:40.057076Z",
"contact": null,
"ucd": "phot.flux;em.UV.100-200nm;stat.min",
"unit": "microJy"
},
{
"id": 369,
"name": "FUVMAGLIMIT10",
"pretty_name": null,
"description": "S/N=10 FUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.531328Z",
"updated": "2021-02-09T04:07:40.069631Z",
"contact": null,
"ucd": "phot.mag;em.UV.100-200nm;stat.min",
"unit": "mag"
},
{
"id": 370,
"name": "FUVMAGLIMIT2p5",
"pretty_name": null,
"description": "S/N=2.5 FUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.549810Z",
"updated": "2021-02-09T04:07:40.099142Z",
"contact": null,
"ucd": "phot.mag;em.UV.100-200nm;stat.min",
"unit": "mag"
},
{
"id": 372,
"name": "NUVFLUXLIMIT10",
"pretty_name": null,
"description": "S/N=10 NUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.592507Z",
"updated": "2021-02-09T04:07:40.151798Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm;stat.min",
"unit": "microJy"
},
{
"id": 373,
"name": "NUVFLUXLIMIT2p5",
"pretty_name": null,
"description": "S/N=2.5 NUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.617386Z",
"updated": "2021-02-09T04:07:40.172194Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm;stat.min",
"unit": "microJy"
},
{
"id": 374,
"name": "NUVFLUXLIMIT5",
"pretty_name": null,
"description": "S/N=5 NUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.644227Z",
"updated": "2021-02-09T04:07:40.193089Z",
"contact": null,
"ucd": "phot.flux;em.UV.200-300nm;stat.min",
"unit": "microJy"
},
{
"id": 375,
"name": "NUVMAGLIMIT10",
"pretty_name": null,
"description": "S/N=10 NUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.660906Z",
"updated": "2021-02-09T04:07:40.206088Z",
"contact": null,
"ucd": "phot.mag;em.UV.200-300nm;stat.min",
"unit": "mag"
},
{
"id": 376,
"name": "NUVMAGLIMIT2p5",
"pretty_name": null,
"description": "S/N=2.5 NUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.677353Z",
"updated": "2021-02-09T04:07:40.218063Z",
"contact": null,
"ucd": "phot.mag;em.UV.200-300nm;stat.min",
"unit": "mag"
},
{
"id": 377,
"name": "NUVMAGLIMIT5",
"pretty_name": null,
"description": "S/N=5 NUV flux detection limit for a circular source at this position",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.702522Z",
"updated": "2021-02-09T04:07:40.231931Z",
"contact": null,
"ucd": "phot.mag;em.UV.200-300nm;stat.min",
"unit": "mag"
},
{
"id": 378,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS objid",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:04.723273Z",
"updated": "2021-02-09T04:07:40.244551Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
}
]
}
]
},
{
"id": 8,
"name": "GroupFinding",
"pretty_name": "GroupFinding",
"description": "This DMU provides the GAMA Galaxy Group Catalogue (G3C).",
"documentation": "GroupFinding<br>2012-07-26<br>Aaron Robotham <asgr@st-and.ac.uk><br><br>The GAMA Galaxy Group Catalogue (G3C) is one of the major data<br>products for the GAMA project. At the most basic level it is a<br>Friends-of-Friends (FoF) group catalogue that has been run on GAMA<br>survey style mocks (put together by Peder Norberg and various<br>collaborators in Durham) to test the quality of the grouping and then<br>run on the real GAMA data in order to extract our best effort<br>groups. The details of the process are discussed extensively in<br><a href=\"http://adsabs.harvard.edu/abs/2011MNRAS.416.2640R\">Robotham et al. 2011 (MNRAS)</a>. <br><br>Note that this release only covers the GAMA G15 survey region, as this<br>is the only region for which DR2 includes data down to the survey<br>limit (r < 19.4 mag).<br><br>This DMU necessarily produces a large number of catalogues and it<br>might seem over-whelming at a glance, but a lot of effort has gone<br>into to simplifying the outputs as much as possible, and limiting the<br>products to the most useful subset of data. The major products are<br>split into the mock groups and the observed GAMA groups. Below we<br>discuss the catalogues contained in the DMU. For most user purposes<br>G3CGal and G3CFoFGroup will be the most useful catalogues.<br><br>For all catalogues the null value is -999 unless stated otherwise.<br><br>The GroupFinding DMU does not have many catalogue dependencies, it<br>only really needs SDSS photometry, RA, DEC, and redshift. The DMUs<br>used to create the GroupFinding DMU are:<br><br>Mocks\t\tv02 (not a GAMA accessible DMU)<br>SpecCat\t v06<br>InputCat v11<br><br>Note that the SpecCat and InputCat versions used here are slightly<br>earlier versions than the ones being released in DR2 (v08 and v16,<br>respectively). The difference between these versions is the addition<br>of more re-redshifting data (see the notes of the SpecCat DMU for an<br>explanation of \"re-redshifting\"). That means that for some objects the<br>redshift and redshift quality used in this DMU will be different from<br>those listed by the SpecCat DMU or in TilingCat.<br><br>-----------------------------------------------------------------------<br><br>G3C GAMA group catalogues:<br><br>G3CGal:<br>List of all galaxies that were used for GAMA grouping. The sample<br>covers the G15 survey region only (r < 19.4 mag) and was selected to<br>be between 0.01 < z < 0.5 to avoid LF and distance uncertainties at<br>very low redshift. This catalogue also contains the group references<br>for grouped galaxies.<br><br>G3CFoFGroup:<br>List of FoF group properties. The GroupID references in G3CGal link to<br>this catalogue.<br><br>G3CLink:<br>List of all galaxy-galaxy links found when running the FoF that<br>created G3CFoFGroup. This is useful if the user wished to know which<br>galaxies are linked the most with other galaxies within a group, or to<br>find the most tenuously associated galaxies within a group.<br><br>G3CGalsInPair:<br>A list of all galaxies that are paired with another galaxy within a<br>projected physical separation of 50 kpc/h and a velocity separation of<br>1,000 km/s. Users should be aware that pairs are listed in both<br>gal1-gal2 and gal2-gal1 combinations, so the number of pairs is half<br>the number of links in this catalogue.<br><br>-------------------------------------------------------------------------<br><br>G3C Mock catalogues:<br><br>9 mock catalogues were created in all, where each mock catalogue<br>covers not only the G15 region as is the case for the real data above,<br>but contains a complete analogue of the full GAMA I survey - i.e. 3<br>regions of 12 x 4 deg^2 out to redshift 0.5. Since the 3 regions have<br>the same size and shape this means that the mocks provide a total of 9<br>x 3 = 27 comparison volumes. The mocks are limited to r < 19.4 mag as<br>are the real data. Each catalogue below contains all 9 mock volumes,<br>with a column specifying the relevant volume number.<br><br>G3CMockGal:<br>List of all galaxies that were used for mock grouping. The sample was<br>selected to be between 0.01 < z < 0.5 to be consistent with the cuts<br>made for the real data. This catalogue also contains the group<br>references for grouped galaxies.<br><br>G3CMockFoFGroup:<br>List of FoF group properties for the mocks. The GroupID references in<br>G3CMockGal link to this catalogue.<br><br>G3CMockHaloGroup:<br>List of halo group properties for the mocks. \"Halo group\" refers to<br>the intrinsic group of galaxies that are given in the mock catalogues,<br>so these groups can be considered to be \"the truth\" for comparison<br>purposes. The HaloID references in G3CMockGal link to this<br>catalogue.<br><br>G3CMockLink:<br>List of all mock galaxy-galaxy links found when running the FoF that<br>created G3CMockFoFGroup. This is useful if the user wishes to know<br>which galaxies are linked the most with other galaxies within a group,<br>or to find the most tenuously associated galaxies within a group.<br><br>G3CMockGalsInPair:<br>A list of all mock galaxies that are paired with another mock galaxy<br>within a projected physical separation of 50 kpc/h and a velocity<br>separation of 1,000 km/s. Users should be aware that pairs are listed<br>in both gal1-gal2 and gal2-gal1 combinations, so the number of pairs<br>is half the number of links in this catalogue.<br><br>",
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"type": "CatalogueGroup",
"created": "2021-01-28T00:39:52.997992Z",
"updated": "2021-02-09T04:07:34.460700Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"tables": [
{
"id": 16,
"name": "G3CGal",
"pretty_name": null,
"description": "Catalogue of all GAMA galaxies used in the G3C. G15 only.",
"documentation": "",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/G3CGal.fits",
"file_name": "G3CGal.fits",
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"version": "v05",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.662975Z",
"updated": "2021-02-09T04:07:34.839057Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"input_cat": false,
"columns": [
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"id": 544,
"name": "CATAID",
"pretty_name": null,
"description": "GAMA ID",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:08.363411Z",
"updated": "2021-02-09T04:07:42.787713Z",
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{
"id": 545,
"name": "DEC",
"pretty_name": null,
"description": "Declination (J2000)",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:08.398677Z",
"updated": "2021-02-09T04:07:42.801068Z",
"contact": null,
"ucd": "pos.eq.dec",
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},
{
"id": 546,
"name": "DM_100_25_75",
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"description": "Distance modulus using H0=100 km/s/Mpc, Omega_m=0.25 and Omega_L=0.75",
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"created": "2021-01-28T00:40:08.433755Z",
"updated": "2021-02-09T04:07:42.813371Z",
"contact": null,
"ucd": "-",
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},
{
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"name": "GroupID",
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"description": "GroupID of the group this galaxy belongs to as listed in G3CFoFGroup, 0 is un-grouped",
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"name": "RA",
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"created": "2021-01-28T00:40:08.472627Z",
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},
{
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"name": "Rpetro",
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"description": "Petrosian apparent r-band magnitude (AB, extinction corrected) [GAMA selection magnitude]",
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},
{
"id": 550,
"name": "SURVEY_CODE",
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"description": "Source of the redshift. See the notes of table TilingCat in the InputCat DMU for full details",
"documentation": "",
"file_path": null,
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"version": null,
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"created": "2021-01-28T00:40:08.512303Z",
"updated": "2021-02-09T04:07:42.877532Z",
"contact": null,
"ucd": "-",
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},
{
"id": 551,
"name": "SigErr",
"pretty_name": null,
"description": "Velocity uncertainty (on redshift): assumed to be 30 km/s for SDSS, 50 km/s for GAMA and 80 km/s for 2dFGRS",
"documentation": "",
"file_path": null,
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"updated": "2021-02-09T04:07:42.889069Z",
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{
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"name": "Z",
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"description": "Heliocentric redshift",
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},
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"name": "G3CGalsInPair",
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"description": "Catalogue of galaxies that live in pairs (thus gal1-gal2 and gal2-gal1 combinations are both listed). Galaxy pairs are required to be within 50 kpc/h in physical separation and 1000 km/s in velocity separation. G15 only.",
"documentation": "",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/G3CGalsInPair.fits",
"file_name": "G3CGalsInPair.fits",
"file_extension": "fits",
"version": "v04",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.698018Z",
"updated": "2021-02-09T04:07:34.850631Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"input_cat": false,
"columns": [
{
"id": 553,
"name": "Gal1CATAID",
"pretty_name": null,
"description": "GAMA ID of galaxy 1 in G3CGal",
"documentation": "",
"file_path": null,
"file_name": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:08.581281Z",
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},
{
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"name": "Gal2CATAID",
"pretty_name": null,
"description": "GAMA ID of galaxy 2 in G3CGal",
"documentation": "",
"file_path": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:08.601317Z",
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"contact": null,
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{
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"name": "PairID",
"pretty_name": null,
"description": "Unique pair ID for catalogue",
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"file_path": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:08.623459Z",
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{
"id": 556,
"name": "SepProjAng",
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"description": "Physical projected separation between galaxy 1 and galaxy 2",
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"created": "2021-01-28T00:40:08.643831Z",
"updated": "2021-02-09T04:07:42.956211Z",
"contact": null,
"ucd": "-",
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},
{
"id": 557,
"name": "SepVel",
"pretty_name": null,
"description": "Velocity separation of galaxy 1 and galaxy 2",
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"file_path": null,
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"created": "2021-01-28T00:40:08.681078Z",
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"contact": null,
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}
]
},
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"name": "G3CFoFGroup",
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"description": "This is a catalogue of G3C GAMA group properties. G15 only.",
"documentation": "GroupFinding<br>G3CFoFGroup<br>v04<br>2011-09-14<br>Aaron Robotham <asgr@st-and.ac.uk><br><br>The cosmology used is H_0=100 km/s/Mpc, Omega_L=0.75,Omega_M=0.25.<br><br>All r-band derived quantities use Rpetro in G3CGal.<br><br>General notes:<br>=============<br><br>a. To obtain a proper total dynamical mass calibration for the groups<br> the user should read section 4.3 in the accompanying paper<br> (Robotham et al. 2011). In the present catalogue, MassProxy<br> is listed with A=1. For Nfof>=5 the suggested best median global<br> correction for the *user to apply* is A=10.0. This is used in the<br> MassA column.<br><br>b. To obtain a proper total luminosity calibration for the groups the<br> user should read section 4.4 in the accompanying paper (Robotham et<br> al. 2011). In the present catalogue, TotFluxProxy is listed<br> with B=1. For Nfof>=5 the suggested best median global correction<br> for the *user to apply* is B=1.04. This is used in the MassB<br> column.<br><br>c. To obtain a proper total (dynamical) mass calibration for the<br> groups from their total luminosity the user should calibrate the<br> luminosity-mass relation independently for the data and the<br> mocks. This calibration should be done using TotFluxProxy (with the<br> appropriate B factor) and MassProxy (with the appropriate A<br> factor). We would generally recommend a median unbiased calibration,<br> split as function of Nfof and Zfof as has been done in Robotham<br> et al. (2011) for most group properties.<br><br>d. To avoid any edge effects, only groups with GroupEdge=1 should be<br> selected. To create a volume limited sample just select the RA and<br> DEC ranges that don't include any groups that have a GroupEdge less<br> than 1.<br><br>e. The final four columns (MassA, MassAfunc, LumMassB and LumMassBfunc)<br> contain the best effort group mass/luminosity scalings. The<br> functional form using the group redshift and multiplicity has<br> the \"func\" suffix, and the global median correction does not.<br>",
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"version": "v04",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.635335Z",
"updated": "2021-02-09T04:07:34.827812Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"input_cat": false,
"columns": [
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"id": 519,
"name": "LinkTot",
"pretty_name": null,
"description": "Total number of FoF links in the system",
"documentation": "",
"file_path": null,
"file_name": null,
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"created": "2021-01-28T00:40:07.696454Z",
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"contact": null,
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"name": "LumB",
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"description": "TotFluxProxy times the global B factor required to get a median unbaised halo mass estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)",
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"file_path": null,
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"created": "2021-01-28T00:40:07.713511Z",
"updated": "2021-02-09T04:07:42.427279Z",
"contact": null,
"ucd": "-",
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},
{
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"name": "LumBfunc",
"pretty_name": null,
"description": "TotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)",
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"file_path": null,
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"created": "2021-01-28T00:40:07.729864Z",
"updated": "2021-02-09T04:07:42.447475Z",
"contact": null,
"ucd": "-",
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},
{
"id": 525,
"name": "Modality",
"pretty_name": null,
"description": "The modality of the system: (1+VelSkew^2)/(3+VelKurt^2). This will be 1/3 for a normal distribution and 0.555 for a uniform.",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:07.821760Z",
"updated": "2021-02-09T04:07:42.494351Z",
"contact": null,
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},
{
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"name": "BCGRA",
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"description": "RA of BCG (J2000)",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:07.470842Z",
"updated": "2021-02-09T04:07:42.207523Z",
"contact": null,
"ucd": "pos.eq.ra",
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},
{
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"name": "AxAng",
"pretty_name": null,
"description": "Angle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:07.402415Z",
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"contact": null,
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{
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"description": "Axial ratio of the group using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)",
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{
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"description": "GAMA ID of BCG",
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"description": "Dec of BCG (J2000)",
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"created": "2021-01-28T00:40:07.453548Z",
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"ucd": "pos.eq.dec",
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},
{
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"name": "CenDec",
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"description": "Dec of group for a r-band luminosity weighted CoM of the system (J2000)",
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},
{
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"description": "RA of group for a r-band luminosity weighted CoM of the system (J2000)",
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},
{
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"description": "Fraction of the group within the survey volume, as estimated from IterCen and Rad100",
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{
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"description": "Unique group ID, as used in G3CGal",
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"created": "2021-01-28T00:40:07.545875Z",
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{
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"name": "IterCenCATAID",
"pretty_name": null,
"description": "GAMA ID of the iterative central galaxy (prefered position of the group centre, see Robotham et al. 2011 section 4.2)",
"documentation": "",
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"pretty_name": null,
"description": "Dec of the iterative central galaxy (J2000)",
"documentation": "",
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"created": "2021-01-28T00:40:07.584662Z",
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{
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"description": "RA of the iterative central galaxy (J2000)",
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{
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"description": "Redshift of the iterative central galaxy",
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},
{
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"description": "Link strength combined, average of LinkStrenProj*LinkStrenZ for all the links in the group (0<=LinkStrenComb<=1)",
"documentation": "",
"file_path": null,
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},
{
"id": 517,
"name": "LinkStrenProj",
"pretty_name": null,
"description": "Link strength in projection, average projected FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenProj<=1)",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:07.659950Z",
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"contact": null,
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},
{
"id": 518,
"name": "LinkStrenRad",
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"version": "v04",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.813374Z",
"updated": "2021-02-09T04:07:34.898890Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"input_cat": false,
"columns": [
{
"id": 616,
"name": "Gal1GalID",
"pretty_name": null,
"description": "GalID of galaxy 1 in G3CMockGal",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.482177Z",
"updated": "2021-02-09T04:07:43.804168Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 617,
"name": "Gal2GalID",
"pretty_name": null,
"description": "GalID of galaxy 2 in G3CMockGal",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.501658Z",
"updated": "2021-02-09T04:07:43.817422Z",
"contact": null,
"ucd": "meta.id",
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},
{
"id": 618,
"name": "PairID",
"pretty_name": null,
"description": "Unique pair ID for catalogue",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.520532Z",
"updated": "2021-02-09T04:07:43.830346Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 619,
"name": "SepProjAng",
"pretty_name": null,
"description": "Physical projected separation between galaxy 1 and galaxy 2",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.537895Z",
"updated": "2021-02-09T04:07:43.842210Z",
"contact": null,
"ucd": "-",
"unit": "kpc/h"
},
{
"id": 620,
"name": "SepVel",
"pretty_name": null,
"description": "Velocity separation of galaxy 1 and galaxy 2",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.581752Z",
"updated": "2021-02-09T04:07:43.871796Z",
"contact": null,
"ucd": "-",
"unit": "km/s"
},
{
"id": 621,
"name": "Volume",
"pretty_name": null,
"description": "The mock volume number",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.623535Z",
"updated": "2021-02-09T04:07:43.882996Z",
"contact": null,
"ucd": "-",
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}
]
},
{
"id": 19,
"name": "G3CMockFoFGroup",
"pretty_name": null,
"description": "This is a catalogue of G3C mock FoF group properties.",
"documentation": "GroupFinding<br>G3CMockFoFGroup<br>v04<br>2011-09-14<br>Aaron Robotham <asgr@st-and.ac.uk><br><br>The cosmology used is H_0=100*h,Omega_L=0.75,Omega_M=0.25.<br><br>All r-band derived quantities use Rpetro in G3CMockGal.<br><br>General notes:<br>=============<br><br>a. To obtain a proper total dynamical mass calibration for the groups<br> the user should read section 4.3 in the accompanying paper<br> (Robotham et al. 2011). In the present catalogue, MassProxy<br> is listed with A=1. For Nfof>=5 the suggested best median global<br> correction for the *user to apply* is A=10.0. This is used in the<br> MassA column.<br><br>b. To obtain a proper total luminosity calibration for the groups the<br> user should read section 4.4 in the accompanying paper (Robotham et<br> al. 2011). In the present catalogue, TotFluxProxy is listed<br> with B=1. For Nfof>=5 the suggested best median global correction<br> for the *user to apply* is B=1.04. This is used in the MassB<br> column.<br><br>c. To obtain a proper total (dynamical) mass calibration for the<br> groups from their total luminosity the user should calibrate the<br> luminosity-mass relation independently for the data and the<br> mocks. This calibration should be done using TotFluxProxy (with the<br> appropriate B factor) and MassProxy (with the appropriate A<br> factor). We would generally recommend a median unbiased calibration,<br> split as function of Nfof and Zfof as has been done in Robotham<br> et al. (2011) for most group properties.<br><br>d. To avoid any edge effects, only groups with GroupEdge=1 should be<br> selected. To create a volume limited sample just select the RA and<br> DEC ranges that don't include any groups that have a GroupEdge less<br> than 1.<br><br>e. The final four columns (MassA, MassAfunc, LumMassB and LumMassBfunc)<br> contain the best effort group mass/luminosity scalings. The<br> functional form using the group redshift and multiplicity has<br> the \"func\" suffix, and the global median correction does not.<br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/G3CMockFoFGroup.fits",
"file_name": "G3CMockFoFGroup.fits",
"file_extension": "fits",
"version": "v04",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.761466Z",
"updated": "2021-02-09T04:07:34.873947Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"input_cat": false,
"columns": [
{
"id": 566,
"name": "AxRat",
"pretty_name": null,
"description": "Axial ratio of the group using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.079844Z",
"updated": "2021-02-09T04:07:43.123926Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 567,
"name": "BCGDec",
"pretty_name": null,
"description": "Dec of BCG (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.106980Z",
"updated": "2021-02-09T04:07:43.136215Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 565,
"name": "AxAng",
"pretty_name": null,
"description": "Angle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.057919Z",
"updated": "2021-02-09T04:07:43.112145Z",
"contact": null,
"ucd": "-",
"unit": "deg"
},
{
"id": 568,
"name": "BCGGalID",
"pretty_name": null,
"description": "GalID of BCG",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.125474Z",
"updated": "2021-02-09T04:07:43.148359Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 569,
"name": "BCGRA",
"pretty_name": null,
"description": "RA of BCG (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.145703Z",
"updated": "2021-02-09T04:07:43.160868Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 570,
"name": "CenDec",
"pretty_name": null,
"description": "Dec of group for a r-band luminosity weighted CoM of the system (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.166182Z",
"updated": "2021-02-09T04:07:43.173411Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 571,
"name": "CenRA",
"pretty_name": null,
"description": "RA of group for a r-band luminosity weighted CoM of the system (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.186994Z",
"updated": "2021-02-09T04:07:43.186413Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 572,
"name": "GroupEdge",
"pretty_name": null,
"description": "Fraction of the group within the survey volume, as estimated from IterCen and Rad100",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.205852Z",
"updated": "2021-02-09T04:07:43.198216Z",
"contact": null,
"ucd": "-",
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},
{
"id": 573,
"name": "GroupID",
"pretty_name": null,
"description": "Unique group ID, as referred to by G3CMockGal",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.224665Z",
"updated": "2021-02-09T04:07:43.210436Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 574,
"name": "IterCenDEC",
"pretty_name": null,
"description": "Dec of the iterative central galaxy (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.252861Z",
"updated": "2021-02-09T04:07:43.224258Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 575,
"name": "IterCenGalID",
"pretty_name": null,
"description": "GalID of the iterative central galaxy (prefered position of the group centre, see Robotham et al. 2011 section 4.2)",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.271507Z",
"updated": "2021-02-09T04:07:43.236997Z",
"contact": null,
"ucd": "meta.id",
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},
{
"id": 576,
"name": "IterCenRA",
"pretty_name": null,
"description": "RA of the iterative central galaxy (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.289513Z",
"updated": "2021-02-09T04:07:43.249077Z",
"contact": null,
"ucd": "pos.eq.ra",
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},
{
"id": 577,
"name": "IterCenZ",
"pretty_name": null,
"description": "Redshift of the iterative central galaxy",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.316738Z",
"updated": "2021-02-09T04:07:43.261990Z",
"contact": null,
"ucd": "-",
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},
{
"id": 578,
"name": "LinkStrenComb",
"pretty_name": null,
"description": "Link strength combined, average of LinkStrenProj*LinkStrenZ for all the links in the group (0<=LinkStrenComb<=1)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.369384Z",
"updated": "2021-02-09T04:07:43.274607Z",
"contact": null,
"ucd": "-",
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},
{
"id": 579,
"name": "LinkStrenProj",
"pretty_name": null,
"description": "Link strength in projection, average projected FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenProj<=1)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
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"created": "2021-01-28T00:40:09.428207Z",
"updated": "2021-02-09T04:07:43.288475Z",
"contact": null,
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},
{
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"name": "LinkStrenRad",
"pretty_name": null,
"description": "Link strength radially, average radial FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenZ<=1)",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
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"created": "2021-01-28T00:40:09.471734Z",
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"contact": null,
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},
{
"id": 581,
"name": "LinkTot",
"pretty_name": null,
"description": "Total number of FoF links in the system",
"documentation": "",
"file_path": null,
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"version": null,
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"created": "2021-01-28T00:40:09.509069Z",
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"contact": null,
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{
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"name": "LumB",
"pretty_name": null,
"description": "TotFluxProxy times the global B factor required to get a median unbaised halo mass estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)",
"documentation": "",
"file_path": null,
"file_name": null,
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"created": "2021-01-28T00:40:09.538356Z",
"updated": "2021-02-09T04:07:43.325485Z",
"contact": null,
"ucd": "-",
"unit": "Lsun"
},
{
"id": 583,
"name": "LumBfunc",
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"description": "TotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:09.582573Z",
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"contact": null,
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},
{
"id": 584,
"name": "MassA",
"pretty_name": null,
"description": "Mass proxy times the global A factor required to get a median unbaised halo mass estimate (A=10.0, see Robotham et al. 2011 section 4.3 for details)",
"documentation": "",
"file_path": null,
"file_name": null,
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"created": "2021-01-28T00:40:09.601982Z",
"updated": "2021-02-09T04:07:43.367546Z",
"contact": null,
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"unit": "Msun"
},
{
"id": 585,
"name": "MassAfunc",
"pretty_name": null,
"description": "Mass proxy times the functional A factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.3 for details)",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:09.628590Z",
"updated": "2021-02-09T04:07:43.379887Z",
"contact": null,
"ucd": "-",
"unit": "Msun"
},
{
"id": 586,
"name": "MassProxy",
"pretty_name": null,
"description": "Proxy for dynamical group mass estimated via M propto Rad50 * VelDisp^2 . Value listed corresponds to A=1 in Eq. 18 of Robotham et al. (2011), i.e. calibrated mass is given by A*M, with A the scaling factor described in section 4.3 of Robotham et al. (2011)",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:09.671224Z",
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"contact": null,
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"unit": "Msun"
},
{
"id": 587,
"name": "Modality",
"pretty_name": null,
"description": "The modality of the system: (1+VelSkew^2)/(3+VelKurt^2). This will be 1/3 for a normal distribution and 0.555 for a uniform.",
"documentation": "",
"file_path": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.717096Z",
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"contact": null,
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{
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"name": "Nfof",
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"description": "Group multiplicity",
"documentation": "",
"file_path": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.760828Z",
"updated": "2021-02-09T04:07:43.416234Z",
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{
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"name": "Rad100",
"pretty_name": null,
"description": "Group radius defined by the most distant group member, based on the projected distance away from IterCenID",
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"created": "2021-01-28T00:40:09.787350Z",
"updated": "2021-02-09T04:07:43.427951Z",
"contact": null,
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"unit": "Mpc/h"
},
{
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"pretty_name": null,
"description": "Group radius defined by the 68th percentile group member, based on the projected distance away from IterCenID",
"documentation": "",
"file_path": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.804991Z",
"updated": "2021-02-09T04:07:43.447423Z",
"contact": null,
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"unit": "Mpc/h"
},
{
"id": 591,
"name": "Rad50",
"pretty_name": null,
"description": "Group radius defined by the 50th percentile group member, based on the projected distance away from IterCenID",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.833276Z",
"updated": "2021-02-09T04:07:43.458715Z",
"contact": null,
"ucd": "-",
"unit": "Mpc/h"
},
{
"id": 592,
"name": "RadKurt",
"pretty_name": null,
"description": "Unbiased kurtosis of the radial distribution of galaxies based on the projected distance to IterCen",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.853437Z",
"updated": "2021-02-09T04:07:43.478059Z",
"contact": null,
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},
{
"id": 593,
"name": "RelDen",
"pretty_name": null,
"description": "Relative galaxy space density (w.r.t. the SWML prediction) within a cylinder of radius 1.5 Mpc/h and length 18Mpc/h centred on IterCenID.",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:09.871703Z",
"updated": "2021-02-09T04:07:43.498267Z",
"contact": null,
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},
{
"id": 594,
"name": "Rgap",
"pretty_name": null,
"description": "Apparent r-band magnitude gap between BCG and second brightest group member",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.889333Z",
"updated": "2021-02-09T04:07:43.510031Z",
"contact": null,
"ucd": "-",
"unit": "mag"
},
{
"id": 595,
"name": "SymKS",
"pretty_name": null,
"description": "KS test of the uniformity of groups once corrected for the axial-ratio; an elliptical group has an average p-value of 0.5 (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.908371Z",
"updated": "2021-02-09T04:07:43.521292Z",
"contact": null,
"ucd": "-",
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},
{
"id": 596,
"name": "TotFluxProxy",
"pretty_name": null,
"description": "Proxy for group total r-band luminosity down to M_r - 5 log_10 h = -14 in solar luminosities. It is based on the total observed r-band flux and the fraction of light (as estimated from the global galaxy LF) observable at the group redshift. Value listed corresponds to B=1 in Eq. 21 of Robotham et al. (2011)",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.927328Z",
"updated": "2021-02-09T04:07:43.541133Z",
"contact": null,
"ucd": "-",
"unit": "Lsun"
},
{
"id": 597,
"name": "TotRmag",
"pretty_name": null,
"description": "r-band absolute magnitude of the group, obtained by adding up the r-band luminosities of its members",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.947380Z",
"updated": "2021-02-09T04:07:43.561201Z",
"contact": null,
"ucd": "-",
"unit": "mag"
},
{
"id": 598,
"name": "VelDisp",
"pretty_name": null,
"description": "Group velocity dispersion, corrected for the total group velocity dispersion error (VelErr); set to zero if VelErr>VelDispRaw (see eq. 17 in Robotham et al. 2011)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:09.965391Z",
"updated": "2021-02-09T04:07:43.573445Z",
"contact": null,
"ucd": "-",
"unit": "km/s"
},
{
"id": 599,
"name": "VelDispRaw",
"pretty_name": null,
"description": "Raw group velocity dispersion",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.003182Z",
"updated": "2021-02-09T04:07:43.584952Z",
"contact": null,
"ucd": "-",
"unit": "km/s"
},
{
"id": 600,
"name": "VelErr",
"pretty_name": null,
"description": "Total group velocity error",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.033024Z",
"updated": "2021-02-09T04:07:43.603307Z",
"contact": null,
"ucd": "-",
"unit": "km/s"
},
{
"id": 601,
"name": "VelKurt",
"pretty_name": null,
"description": "Unbiased kurtosis of the galaxy velocities (requires 4 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.076601Z",
"updated": "2021-02-09T04:07:43.615418Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 602,
"name": "VelSkew",
"pretty_name": null,
"description": "Unbiased skew of the galaxy velocities (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.120336Z",
"updated": "2021-02-09T04:07:43.629473Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 603,
"name": "Volume",
"pretty_name": null,
"description": "The mock volume number",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.165238Z",
"updated": "2021-02-09T04:07:43.647766Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 604,
"name": "Zfof",
"pretty_name": null,
"description": "Median redshift of the group",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.209928Z",
"updated": "2021-02-09T04:07:43.658907Z",
"contact": null,
"ucd": "-",
"unit": "-"
}
]
},
{
"id": 22,
"name": "G3CMockHaloGroup",
"pretty_name": null,
"description": "This is a catalogue of G3C mock halo group properties. These are the intrinsic groups found in the mocks.",
"documentation": "GroupFinding<br>G3CMockHaloGroup<br>v04<br>2011-09-14<br>Aaron Robotham <asgr@st-and.ac.uk><br><br>This catalogue contains the \"true\" groups found in the mock<br>simulations. This can be used for comparison purposes to test the<br>quality of the FoF grouping.<br><br>The cosmology used is H_0=100*h,Omega_L=0.75,Omega_M=0.25.<br><br>All r-band derived quantities use Rpetro in G3CMockGal.<br><br>General notes:<br>=============<br><br>a. To obtain a proper total dynamical mass calibration for the groups<br> the user should read section 4.3 in the accompanying paper<br> (Robotham et al. 2011). In the present catalogue, MassProxy<br> is listed with A=1. For Nfof>=5 the suggested best median global<br> correction for the *user to apply* is A=10.0. This is used in the<br> MassA column.<br><br>b. To obtain a proper total luminosity calibration for the groups the<br> user should read section 4.4 in the accompanying paper (Robotham et<br> al. 2011). In the present catalogue, TotFluxProxy is listed<br> with B=1. For Nfof>=5 the suggested best median global correction<br> for the *user to apply* is B=1.04. This is used in the MassB<br> column.<br><br>c. To obtain a proper total (dynamical) mass calibration for the<br> groups from their total luminosity the user should calibrate the<br> luminosity-mass relation independently for the data and the<br> mocks. This calibration should be done using TotFluxProxy (with the<br> appropriate B factor) and MassProxy (with the appropriate A<br> factor). We would generally recommend a median unbiased calibration,<br> split as function of Nfof and Zfof as has been done in Robotham<br> et al. (2011) for most group properties.<br><br>d. To avoid any edge effects, only groups with GroupEdge=1 should be<br> selected. To create a volume limited sample just select the RA and<br> DEC ranges that don't include any groups that have a GroupEdge less<br> than 1.<br><br>e. The final four columns (MassA, MassAfunc, LumMassB and LumMassBfunc)<br> contain the best effort group mass/luminosity scalings. The<br> functional form using the group redshift and multiplicity has<br> the \"func\" suffix, and the global median correction does not.<br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/G3CMockHaloGroup.fits",
"file_name": "G3CMockHaloGroup.fits",
"file_extension": "fits",
"version": "v04",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.829523Z",
"updated": "2021-02-09T04:07:34.911391Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"input_cat": false,
"columns": [
{
"id": 654,
"name": "VelErr",
"pretty_name": null,
"description": "Total group velocity error",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.689168Z",
"updated": "2021-02-09T04:07:44.416623Z",
"contact": null,
"ucd": "-",
"unit": "km/s"
},
{
"id": 656,
"name": "VelSkew",
"pretty_name": null,
"description": "Unbiased skew of the galaxy velocities (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.784455Z",
"updated": "2021-02-09T04:07:44.439849Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 622,
"name": "AxAng",
"pretty_name": null,
"description": "Angle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.649870Z",
"updated": "2021-02-09T04:07:43.895516Z",
"contact": null,
"ucd": "-",
"unit": "deg"
},
{
"id": 623,
"name": "AxRat",
"pretty_name": null,
"description": "Axial ratio of the group using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.684438Z",
"updated": "2021-02-09T04:07:43.907133Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 624,
"name": "BCGDec",
"pretty_name": null,
"description": "Dec of BCG (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.720271Z",
"updated": "2021-02-09T04:07:43.918791Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 625,
"name": "BCGGalID",
"pretty_name": null,
"description": "GalID of BCG",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.744836Z",
"updated": "2021-02-09T04:07:43.930668Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 626,
"name": "BCGRA",
"pretty_name": null,
"description": "RA of BCG (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.765050Z",
"updated": "2021-02-09T04:07:43.942216Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 627,
"name": "CenDec",
"pretty_name": null,
"description": "Dec of group for a r-band luminosity weighted CoM of the system (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.807227Z",
"updated": "2021-02-09T04:07:43.955154Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 628,
"name": "CenRA",
"pretty_name": null,
"description": "RA of group for a r-band luminosity weighted CoM of the system (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.851582Z",
"updated": "2021-02-09T04:07:43.966986Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 629,
"name": "GroupEdge",
"pretty_name": null,
"description": "Fraction of the group within the survey volume, as estimated from IterCen and Rad100",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.904677Z",
"updated": "2021-02-09T04:07:43.980654Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 630,
"name": "HaloID",
"pretty_name": null,
"description": "Unique halo ID, as referred to by G3CMockGal",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.951153Z",
"updated": "2021-02-09T04:07:43.994157Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 631,
"name": "HaloMass",
"pretty_name": null,
"description": "The dark matter halo mass for the group halo in the Millennium simulation",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:10.987803Z",
"updated": "2021-02-09T04:07:44.007418Z",
"contact": null,
"ucd": "-",
"unit": "Msun/h"
},
{
"id": 632,
"name": "IterCenDEC",
"pretty_name": null,
"description": "Dec of the iterative central galaxy (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.022249Z",
"updated": "2021-02-09T04:07:44.027437Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 633,
"name": "IterCenGalID",
"pretty_name": null,
"description": "GalID of the iterative central galaxy (prefered position of the group centre, see Robotham et al. 2011 section 4.2)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.070923Z",
"updated": "2021-02-09T04:07:44.048333Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 634,
"name": "IterCenRA",
"pretty_name": null,
"description": "RA of the iterative central galaxy (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.097324Z",
"updated": "2021-02-09T04:07:44.069269Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 635,
"name": "IterCenZ",
"pretty_name": null,
"description": "Redshift of the iterative central galaxy",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.115617Z",
"updated": "2021-02-09T04:07:44.082111Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 636,
"name": "LumB",
"pretty_name": null,
"description": "TotFluxProxy times the global B factor required to get a median unbaised halo mass estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.133688Z",
"updated": "2021-02-09T04:07:44.114962Z",
"contact": null,
"ucd": "-",
"unit": "Lsun"
},
{
"id": 637,
"name": "LumBfunc",
"pretty_name": null,
"description": "TotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.152927Z",
"updated": "2021-02-09T04:07:44.138002Z",
"contact": null,
"ucd": "-",
"unit": "Lsun"
},
{
"id": 638,
"name": "MassA",
"pretty_name": null,
"description": "Mass proxy times the global A factor required to get a median unbaised halo mass estimate (A=10.0, see Robotham et al. 2011 section 4.3 for details)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.173194Z",
"updated": "2021-02-09T04:07:44.149923Z",
"contact": null,
"ucd": "-",
"unit": "Msun"
},
{
"id": 639,
"name": "MassAfunc",
"pretty_name": null,
"description": "Mass proxy times the functional A factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.3 for details)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.191701Z",
"updated": "2021-02-09T04:07:44.171019Z",
"contact": null,
"ucd": "-",
"unit": "Msun"
},
{
"id": 640,
"name": "MassProxy",
"pretty_name": null,
"description": "Proxy for dynamical group mass estimated via M propto Rad50 * VelDisp^2 . Value listed corresponds to A=1 in Eq. 18 of Robotham et al. (2011), i.e. calibrated mass is given by A*M, with A the scaling factor described in section 4.3 of Robotham et al. (2011)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.231280Z",
"updated": "2021-02-09T04:07:44.191644Z",
"contact": null,
"ucd": "-",
"unit": "Msun"
},
{
"id": 641,
"name": "Modality",
"pretty_name": null,
"description": "The modality of the system: (1+VelSkew^2)/(3+VelKurt^2). This will be 1/3 for a normal distribution and 0.555 for a uniform.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.249870Z",
"updated": "2021-02-09T04:07:44.212845Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 642,
"name": "Nhalo",
"pretty_name": null,
"description": "Group multiplicity",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.278342Z",
"updated": "2021-02-09T04:07:44.225566Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 643,
"name": "Rad100",
"pretty_name": null,
"description": "Group radius defined by the most distant group member, based on the projected distance away from IterCenID",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.298484Z",
"updated": "2021-02-09T04:07:44.239093Z",
"contact": null,
"ucd": "-",
"unit": "Mpc/h"
},
{
"id": 644,
"name": "Rad1Sig",
"pretty_name": null,
"description": "Group radius defined by the 68th percentile group member, based on the projected distance away from IterCenID",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.327862Z",
"updated": "2021-02-09T04:07:44.251527Z",
"contact": null,
"ucd": "-",
"unit": "Mpc/h"
},
{
"id": 645,
"name": "Rad50",
"pretty_name": null,
"description": "Group radius defined by the 50th percentile group member, based on the projected distance away from IterCenID",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.377142Z",
"updated": "2021-02-09T04:07:44.265144Z",
"contact": null,
"ucd": "-",
"unit": "Mpc/h"
},
{
"id": 646,
"name": "RadKurt",
"pretty_name": null,
"description": "Unbiased kurtosis of the radial distribution of galaxies based on the projected distance to IterCen",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.421082Z",
"updated": "2021-02-09T04:07:44.278412Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 647,
"name": "RelDen",
"pretty_name": null,
"description": "Relative galaxy space density (w.r.t. the SWML prediction) within a cylinder of radius 1.5 Mpc/h and length 18Mpc/h centred on IterCenID.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.441866Z",
"updated": "2021-02-09T04:07:44.302569Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 648,
"name": "Rgap",
"pretty_name": null,
"description": "Apparent r-band magnitude gap between BCG and second brightest group member",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.475343Z",
"updated": "2021-02-09T04:07:44.324040Z",
"contact": null,
"ucd": "-",
"unit": "mag"
},
{
"id": 649,
"name": "SymKS",
"pretty_name": null,
"description": "KS test of the uniformity of groups once corrected for the axial-ratio; an elliptical group has an average p-value of 0.5 (requires 3 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.526735Z",
"updated": "2021-02-09T04:07:44.337646Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 650,
"name": "TotFluxProxy",
"pretty_name": null,
"description": "Proxy for group total r-band luminosity down to M_r - 5 log_10 h = -14 in solar luminosities. It is based on TotFlux and the fraction of light (as estimated from the global galaxy LF) observable at the group redshift. Value listed corresponds to B=1 in Eq. 21 of Robotham et al. (2011)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.553721Z",
"updated": "2021-02-09T04:07:44.349738Z",
"contact": null,
"ucd": "-",
"unit": "Lsun"
},
{
"id": 651,
"name": "TotRmag",
"pretty_name": null,
"description": "Observed r-band absolute magnitude of the group, obtained by adding up the r-band luminosities of its members",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.581889Z",
"updated": "2021-02-09T04:07:44.377771Z",
"contact": null,
"ucd": "-",
"unit": "mag"
},
{
"id": 652,
"name": "VelDisp",
"pretty_name": null,
"description": "Group velocity dispersion, corrected for the total group velocity dispersion error (VelErr); set to zero if VelErr>VelDispRaw (see eq. 17 in Robotham et al. 2011)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.624119Z",
"updated": "2021-02-09T04:07:44.392472Z",
"contact": null,
"ucd": "-",
"unit": "km/s"
},
{
"id": 653,
"name": "VelDispRaw",
"pretty_name": null,
"description": "Raw group velocity dispersion",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.662034Z",
"updated": "2021-02-09T04:07:44.404439Z",
"contact": null,
"ucd": "-",
"unit": "km/s"
},
{
"id": 655,
"name": "VelKurt",
"pretty_name": null,
"description": "Unbiased kurtosis of the galaxy velocities (requires 4 or more members, so -999 otherwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.724208Z",
"updated": "2021-02-09T04:07:44.428508Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 657,
"name": "Volume",
"pretty_name": null,
"description": "The mock volume number",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.813382Z",
"updated": "2021-02-09T04:07:44.451925Z",
"contact": null,
"ucd": "-",
"unit": "-"
},
{
"id": 658,
"name": "Zhalo",
"pretty_name": null,
"description": "Median redshift of the group",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.832665Z",
"updated": "2021-02-09T04:07:44.463673Z",
"contact": null,
"ucd": "-",
"unit": "-"
}
]
},
{
"id": 23,
"name": "G3CMockLink",
"pretty_name": null,
"description": "Catalogue that gives linking between all mock galaxies that share a common group in G3CMockFoFGroup.",
"documentation": "",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/G3CMockLink.fits",
"file_name": "G3CMockLink.fits",
"file_extension": "fits",
"version": "v04",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.863942Z",
"updated": "2021-02-09T04:07:34.931745Z",
"contact": {
"email": "asgr@st-and.ac.uk",
"name": "Aaron Robotham "
},
"input_cat": false,
"columns": [
{
"id": 659,
"name": "Gal1ID",
"pretty_name": null,
"description": "GalID of galaxy 1 in G3CMockGal",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.850950Z",
"updated": "2021-02-09T04:07:44.475019Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 660,
"name": "Gal2ID",
"pretty_name": null,
"description": "GalID of galaxy 2 in G3CMockGal",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.869925Z",
"updated": "2021-02-09T04:07:44.487502Z",
"contact": null,
"ucd": "meta.id",
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},
{
"id": 661,
"name": "LimProjCo",
"pretty_name": null,
"description": "Maximum allowed projected separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimProjCo>=SepProjCo)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.890314Z",
"updated": "2021-02-09T04:07:44.500417Z",
"contact": null,
"ucd": "-",
"unit": "kpc/h"
},
{
"id": 662,
"name": "LimRadCo",
"pretty_name": null,
"description": "Maximum allowed radial separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimRadCo>=SepRadCo)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.909253Z",
"updated": "2021-02-09T04:07:44.512962Z",
"contact": null,
"ucd": "-",
"unit": "kpc/h"
},
{
"id": 663,
"name": "LinkID",
"pretty_name": null,
"description": "Unique linking ID for catalogue",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.929086Z",
"updated": "2021-02-09T04:07:44.525520Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 664,
"name": "SepProjCo",
"pretty_name": null,
"description": "Projected separation of galaxy 1 and galaxy 2 in comoving coordinates",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.948480Z",
"updated": "2021-02-09T04:07:44.538123Z",
"contact": null,
"ucd": "-",
"unit": "kpc/h"
},
{
"id": 665,
"name": "SepRadCo",
"pretty_name": null,
"description": "Radial separation of galaxy 1 and galaxy 2 in comoving coordinates",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.968840Z",
"updated": "2021-02-09T04:07:44.551544Z",
"contact": null,
"ucd": "-",
"unit": "kpc/h"
},
{
"id": 666,
"name": "Volume",
"pretty_name": null,
"description": "The mock volume number",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:11.987868Z",
"updated": "2021-02-09T04:07:44.562879Z",
"contact": null,
"ucd": "-",
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}
]
}
]
},
{
"id": 9,
"name": "InputCat",
"pretty_name": "InputCat",
"description": "This DMU provides various input catalogues for the spectroscopy.",
"documentation": "InputCat<br>2011-07-20<br>Ivan Baldry <ikb@astro.livjm.ac.uk><br><br>This data management unit produces various input catalogues for the<br>GAMA I survey regions. We expect that the table TilingCat will be of<br>most interest to most users.<br>",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v16",
"type": "CatalogueGroup",
"created": "2021-01-28T00:39:53.039352Z",
"updated": "2021-02-09T04:07:34.470475Z",
"contact": {
"email": "ikb@astro.livjm.ac.uk",
"name": "Ivan Baldry "
},
"tables": [
{
"id": 24,
"name": "GalacticExtinction",
"pretty_name": null,
"description": "This table provides the Galactic foreground extinction in all GALEX, SDSS and UKIDSS bands for every object in InputCatA and SpStandards.",
"documentation": "InputCat<br>GalacticExtinction<br>v01<br>2011-12-08<br>Joe Liske <jliske@eso.org><br><br>This table provides the Galactic foreground extinction in all GALEX,<br>SDSS and UKIDSS bands for the position of every object listed in<br>InputCatA and SpStandards.<br><br>The extinction in each band x was calculated as<br>A_x = (A_x / E(B-V)) * E(B-V).<br><br>For each position in this table the value of E(B-V) was taken from the<br>dust maps of <a href=\"http://adsabs.harvard.edu/abs/1998ApJ...500..525S\">Schlegel et al. (1998)</a>, interpolating from the nearest 4<br>pixels.<br><br>The values of A_x/E(B-V) were taken from this list:<br><br>Band A_x/E(B-V)<br>--------------------------<br> GALEX<br>FUV 8.376<br>NUV 8.741<br> MGC<br>B 4.23<br> SDSS<br>u 5.155<br>g 3.793<br>r 2.751<br>i 2.086<br>z 1.479<br> UKIDSS<br>Y 1.211<br>J 0.889<br>H 0.578<br>K 0.360<br><br><br>The SDSS values were taken from <a href=\"http://adsabs.harvard.edu/abs/1998ApJ...500..525S\">Schlegel et al. (1998)</a>. These were<br>calculated assuming the extinction law of <a href=\"http://adsabs.harvard.edu/abs/1994ApJ...422..158O\">O'Donnell (1994)</a> in the<br>optical and that of <a href=\"http://adsabs.harvard.edu/abs/1989ApJ...345..245C\">Cardelli et al. (1989)</a> in the UV and IR, with<br>R_V=3.1, and a z=0 elliptical galaxy spectrum.<br><br>The GALEX values were taken from <a href=\"http://adsabs.harvard.edu/abs/2005ApJ...619L..15W\">Wyder et al. (2005)</a>. These were<br>calculated assuming the extinction law of <a href=\"http://adsabs.harvard.edu/abs/1989ApJ...345..245C\">Cardelli et al. (1989)</a>. The<br>R_V value used in this calculation was not specified. In addition, no<br>source spectrum was used, instead the extinction law was simply<br>averaged over the filter.<br><br>The UKIDSS values were taken from the <a href=\"http://surveys.roe.ac.uk/wsa/\">WFCAM Science Archive</a>. According<br>to Nick Cross these values were calculated assuming the extinction law<br>of <a href=\"http://adsabs.harvard.edu/abs/1989ApJ...345..245C\">Cardelli et al. (1989)</a>, with R_V=3.1, and a z=0 elliptical galaxy<br>spectrum (i.e. exactly following the procedure of <a href=\"http://adsabs.harvard.edu/abs/1998ApJ...500..525S\">Schlegel et<br>al. 1998</a>).<br><br>The MGC value was taken from <a href=\"http://adsabs.harvard.edu/abs/2003MNRAS.344..307L\">Liske et al. (2003)</a>. How this value was<br>calculated is lost in the mists of time.<br><br>Note that the extinction values for the SDSS bands in this table are<br>identical to those provided by the SDSS database (see also <a href=\"http://adsabs.harvard.edu/abs/2002AJ....123..485S\">Stoughton<br>et al. 2002</a>).<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/GalacticExtinction.fits",
"file_name": "GalacticExtinction.fits",
"file_extension": "fits",
"version": "v01",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.899564Z",
"updated": "2021-02-09T04:07:34.942535Z",
"contact": {
"email": "jliske@eso.org",
"name": "Joe Liske "
},
"input_cat": false,
"columns": [
{
"id": 667,
"name": "A_B",
"pretty_name": null,
"description": "Galactic extinction in MGC B band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.007008Z",
"updated": "2021-02-09T04:07:44.575778Z",
"contact": null,
"ucd": "phys.absorption.gal;em.opt.B",
"unit": "mag"
},
{
"id": 668,
"name": "A_FUV",
"pretty_name": null,
"description": "Galactic extinction in GALEX FUV band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.037730Z",
"updated": "2021-02-09T04:07:44.587647Z",
"contact": null,
"ucd": "phys.absorption.gal;em.UV.100-200nm",
"unit": "mag"
},
{
"id": 669,
"name": "A_H",
"pretty_name": null,
"description": "Galactic extinction in UKIDSS H band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.072678Z",
"updated": "2021-02-09T04:07:44.601112Z",
"contact": null,
"ucd": "phys.absorption.gal;em.IR.H",
"unit": "mag"
},
{
"id": 670,
"name": "A_J",
"pretty_name": null,
"description": "Galactic extinction in UKIDSS J band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.122502Z",
"updated": "2021-02-09T04:07:44.625380Z",
"contact": null,
"ucd": "phys.absorption.gal;em.IR.J",
"unit": "mag"
},
{
"id": 671,
"name": "A_K",
"pretty_name": null,
"description": "Galactic extinction in UKIDSS K band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.165512Z",
"updated": "2021-02-09T04:07:44.637888Z",
"contact": null,
"ucd": "phys.absorption.gal;em.IR.K",
"unit": "mag"
},
{
"id": 672,
"name": "A_NUV",
"pretty_name": null,
"description": "Galactic extinction in GALEX NUV band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.209230Z",
"updated": "2021-02-09T04:07:44.651135Z",
"contact": null,
"ucd": "phys.absorption.gal;em.UV.200-300nm",
"unit": "mag"
},
{
"id": 673,
"name": "A_Y",
"pretty_name": null,
"description": "Galactic extinction in UKIDSS Y band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.246873Z",
"updated": "2021-02-09T04:07:44.673333Z",
"contact": null,
"ucd": "phys.absorption.gal;em.IR.NIR",
"unit": "mag"
},
{
"id": 674,
"name": "A_g",
"pretty_name": null,
"description": "Galactic extinction in SDSS g band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.273304Z",
"updated": "2021-02-09T04:07:44.685364Z",
"contact": null,
"ucd": "phys.absorption.gal;em.opt.B",
"unit": "mag"
},
{
"id": 675,
"name": "A_i",
"pretty_name": null,
"description": "Galactic extinction in SDSS i band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.293043Z",
"updated": "2021-02-09T04:07:44.698957Z",
"contact": null,
"ucd": "phys.absorption.gal;em.opt.I",
"unit": "mag"
},
{
"id": 676,
"name": "A_r",
"pretty_name": null,
"description": "Galactic extinction in SDSS r band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.342272Z",
"updated": "2021-02-09T04:07:44.711241Z",
"contact": null,
"ucd": "phys.absorption.gal;em.opt.R",
"unit": "mag"
},
{
"id": 677,
"name": "A_u",
"pretty_name": null,
"description": "Galactic extinction in SDSS u band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.377702Z",
"updated": "2021-02-09T04:07:44.724531Z",
"contact": null,
"ucd": "phys.absorption.gal;em.opt.U",
"unit": "mag"
},
{
"id": 678,
"name": "A_z",
"pretty_name": null,
"description": "Galactic extinction in SDSS z band",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.395718Z",
"updated": "2021-02-09T04:07:44.737101Z",
"contact": null,
"ucd": "phys.absorption.gal;em.opt",
"unit": "mag"
},
{
"id": 679,
"name": "CATAID",
"pretty_name": null,
"description": "Unique GAMA of object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.413390Z",
"updated": "2021-02-09T04:07:44.749337Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 680,
"name": "DEC",
"pretty_name": null,
"description": "DEC of position for which the extinction was calculated (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.433343Z",
"updated": "2021-02-09T04:07:44.761097Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 681,
"name": "EBV",
"pretty_name": null,
"description": "E(B-V)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.455087Z",
"updated": "2021-02-09T04:07:44.772275Z",
"contact": null,
"ucd": "phys.absorption.gal",
"unit": "mag"
},
{
"id": 682,
"name": "RA",
"pretty_name": null,
"description": "RA of position for which the extinction was calculated (J2000)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.472889Z",
"updated": "2021-02-09T04:07:44.783552Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
}
]
},
{
"id": 26,
"name": "SpStandards",
"pretty_name": null,
"description": "Standard stars from SDSS.",
"documentation": "InputCat<br>SpStandards<br>v06<br>2011-01-13<br>Ivan Baldry <ikb@astro.livjm.ac.uk><br><br>This table contains standard stars from SDSS used in GAMA observing.<br>The standard stars can be used to tie the AAOmega spectra to SDSS<br>spectrophotometric calibration, at least in an average sense.<br><br>The standards were selected using the flag sectarget=2 or<br>sectarget=32. The magnitude restrictions were fibermag_r > 16.9 and<br>16.6 < psfmag_r < 18.4. Magnitudes were not extinction corrected.<br><br>priority_class (p):<br><br>p=3: SDSS standard stars with SDSS spectra obtained<br>p=2: classified as SPECTROPHOTO_STD<br>p=1: classified as REDDEN_STD<br>p=0: close proximity to science targets<br><br>See SDSS EDR paper (<a href=\"http://adsabs.harvard.edu/abs/2002AJ....123..485S\">Stoughton et al. 2002</a>, sec 4.8.5).<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/SpStandards.fits",
"file_name": "SpStandards.fits",
"file_extension": "fits",
"version": "v06",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.944760Z",
"updated": "2021-02-09T04:07:34.974096Z",
"contact": {
"email": "ikb@astro.livjm.ac.uk",
"name": "Ivan Baldry "
},
"input_cat": false,
"columns": [
{
"id": 716,
"name": "RA",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.496717Z",
"updated": "2021-02-09T04:07:45.206089Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 717,
"name": "RUN",
"pretty_name": null,
"description": "SDSS run number",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.559757Z",
"updated": "2021-02-09T04:07:45.217776Z",
"contact": null,
"ucd": "obs.param",
"unit": "-"
},
{
"id": 718,
"name": "SECTARGET",
"pretty_name": null,
"description": "2^1 for REDDEN_STD, 2^5 for SPECTROPHOTO_STD",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.607419Z",
"updated": "2021-02-09T04:07:45.230012Z",
"contact": null,
"ucd": "meta.code.class",
"unit": "-"
},
{
"id": 708,
"name": "CATAID",
"pretty_name": null,
"description": "GAMA ID",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.161933Z",
"updated": "2021-02-09T04:07:45.104621Z",
"contact": null,
"ucd": "meta.id;meta.main",
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},
{
"id": 709,
"name": "DEC",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.196941Z",
"updated": "2021-02-09T04:07:45.115958Z",
"contact": null,
"ucd": "pos.eq.dec",
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},
{
"id": 710,
"name": "FIBERMAG_R",
"pretty_name": null,
"description": "DR7 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.260585Z",
"updated": "2021-02-09T04:07:45.127489Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 711,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS ID",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.304552Z",
"updated": "2021-02-09T04:07:45.139952Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 712,
"name": "PRIORITY_CLASS",
"pretty_name": null,
"description": "See notes",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.339450Z",
"updated": "2021-02-09T04:07:45.152438Z",
"contact": null,
"ucd": "meta.code.class",
"unit": "-"
},
{
"id": 713,
"name": "PSFMAG_G",
"pretty_name": null,
"description": "DR7 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.358382Z",
"updated": "2021-02-09T04:07:45.165740Z",
"contact": null,
"ucd": "phot.mag;em.opt",
"unit": "mag"
},
{
"id": 714,
"name": "PSFMAG_I",
"pretty_name": null,
"description": "DR7 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.401978Z",
"updated": "2021-02-09T04:07:45.179773Z",
"contact": null,
"ucd": "phot.mag;em.opt.I",
"unit": "mag"
},
{
"id": 715,
"name": "PSFMAG_R",
"pretty_name": null,
"description": "DR7 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.445642Z",
"updated": "2021-02-09T04:07:45.192362Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 719,
"name": "STATUS",
"pretty_name": null,
"description": "SDSS status flag related to primary secondary",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.634295Z",
"updated": "2021-02-09T04:07:45.241598Z",
"contact": null,
"ucd": "meta.code.status",
"unit": "-"
}
]
},
{
"id": 25,
"name": "InputCatA",
"pretty_name": null,
"description": "SDSS DR6 data of GAMA I survey regions. This is GAMA`s master input catalogue.",
"documentation": "InputCat<br>InputCatA<br>v05<br>2010-05-21<br>Ivan Baldry <ikb@astro.livjm.ac.uk><br><br>This table contains the r_petro < 19.8 SDSS DR6 input catalogue covering<br>an enlarged area (120.0 < RA < 230.0, DEC < 3.0), an r_model < 20.5<br>catalogue covering the three 12x4 GAMA I regions, and a small addition<br>of i_model < 20.5 and FIRST radio matches.<br><br>960510 rows<br><br>The creation of the catalogue is derived from four SQL queries to<br>casjobs DR6. This is the order in which objects were added to this<br>catalogue. The GAMA ID called CATAID runs from 0 to 960509 following<br>the order of these queries.<br><br>..................................................................<br><br>(689669 rows: original version while GAMA regions were still being<br>finalised)<br><br>select ...<br>into ... from dr6.PhotoObj as p<br>where p.psfmag_r - p.modelmag_r > 0.25 and <br> p.petromag_r - p.extinction_r < 19.8 and <br> p.petromag_r - p.extinction_r > 6.0 and<br> p.ra > 120.0 and p.ra < 230.0 and p.dec < 3.0 and<br> ((p.mode = 1) or (p.mode = 2 and p.ra < 139.939 and p.dec < -0.5<br> and (p.status & dbo.fphotostatus('OK_SCANLINE')) > 0))<br><br>Only \"primary\" objects were included except for some \"secondary\"<br>objects along the bottom edge of the equatorial stripe. These really<br>are primary as there are no overlapping stripes. This was necessary<br>for the GAMA 9-h region.<br><br>..................................................................<br><br>(61660 rows: adding in compact objects, only a subset will be<br>targeted)<br><br>...<br>where p.psfmag_r - p.modelmag_r > 0.05 and p.psfmag_r - p.modelmag_r <= 0.25 and<br> p.petromag_r - p.extinction_r < 19.8 and <br> p.petromag_r - p.extinction_r > 6.0 and<br> p.ra > 120.0 and p.ra < 230.0 and p.dec < 3.0 and <br>((p.mode = 1) or (p.mode = 2 and p.ra < 139.939 and p.dec < -0.5<br> and (p.status & dbo.fphotostatus('OK_SCANLINE')) > 0))<br><br>..................................................................<br><br>(208196 rows: adding in objects to r_model < 20.5 in selected regions)<br><br>...<br>where p.psfmag_r - p.modelmag_r > 0.05 and <br> p.modelmag_r - p.extinction_r < 20.5 and<br> p.petromag_r - p.extinction_r >= 19.8 and<br> ( (p.ra > 129.0 and p.ra < 141.0 and p.dec > -1.0 and p.dec < 3.0) or <br> (p.ra > 174.0 and p.ra < 186.0 and p.dec > -2.0 and p.dec < 2.0) or <br> (p.ra > 211.5 and p.ra < 223.5 and p.dec > -2.0 and p.dec < 2.0) ) and <br> ((p.mode = 1) or (p.mode = 2 and p.ra < 139.939 and p.dec < -0.5<br> and (p.status & dbo.fphotostatus('OK_SCANLINE')) > 0))<br><br>..................................................................<br><br>(985 rows: adding in objects to i_model < 20.5 with FIRST radio match)<br><br>...<br>into ... from dr6.PhotoObj as p join dr6.first as f on f.objid = p.objid<br>where p.modelmag_i - p.extinction_i < 20.5 and <br> ( p.psfmag_r - p.modelmag_r <= 0.05 or <br> (p.modelmag_r - p.extinction_r >= 20.5 and<br> p.petromag_r - p.extinction_r >= 19.8) ) and<br> ( (p.ra > 129.0 and p.ra < 141.0 and p.dec > -1.0 and p.dec < 3.0) or <br> (p.ra > 174.0 and p.ra < 186.0 and p.dec > -2.0 and p.dec < 2.0) or <br> (p.ra > 211.5 and p.ra < 223.5 and p.dec > -2.0 and p.dec < 2.0) ) and <br> ((p.mode = 1) or (p.mode = 2 and p.ra < 139.939 and p.dec < -0.5<br> and (p.status & dbo.fphotostatus('OK_SCANLINE')) > 0))<br><br>............................................................................<br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/InputCatA.fits",
"file_name": "InputCatA.fits",
"file_extension": "fits",
"version": "v05",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.926300Z",
"updated": "2021-02-09T04:07:34.954131Z",
"contact": {
"email": "ikb@astro.livjm.ac.uk",
"name": "Ivan Baldry "
},
"input_cat": false,
"columns": [
{
"id": 683,
"name": "CATAID",
"pretty_name": null,
"description": "Unique GAMA ID of object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.490683Z",
"updated": "2021-02-09T04:07:44.795054Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 684,
"name": "DEC",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.510337Z",
"updated": "2021-02-09T04:07:44.806312Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 685,
"name": "EXTINCTION_R",
"pretty_name": null,
"description": "r-band Galactic extinction",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.535982Z",
"updated": "2021-02-09T04:07:44.817821Z",
"contact": null,
"ucd": "phys.absorption.gal;em.opt.R",
"unit": "mag"
},
{
"id": 686,
"name": "FIBERMAG_R",
"pretty_name": null,
"description": "3-arcsec fiber magnitude",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.556284Z",
"updated": "2021-02-09T04:07:44.832164Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 687,
"name": "FLAGS",
"pretty_name": null,
"description": "See SDSS photoobj table",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.574612Z",
"updated": "2021-02-09T04:07:44.843778Z",
"contact": null,
"ucd": "meta.code.qual;phot",
"unit": "-"
},
{
"id": 688,
"name": "FLAGS_R",
"pretty_name": null,
"description": "See SDSS photoobj table",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.601007Z",
"updated": "2021-02-09T04:07:44.855390Z",
"contact": null,
"ucd": "meta.code.qual;phot;em.opt.R",
"unit": "-"
},
{
"id": 689,
"name": "MODELMAG_G",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.620198Z",
"updated": "2021-02-09T04:07:44.867162Z",
"contact": null,
"ucd": "phot.mag;em.opt",
"unit": "mag"
},
{
"id": 690,
"name": "MODELMAG_I",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.655645Z",
"updated": "2021-02-09T04:07:44.884290Z",
"contact": null,
"ucd": "phot.mag;em.opt.I",
"unit": "mag"
},
{
"id": 691,
"name": "MODELMAG_R",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.684743Z",
"updated": "2021-02-09T04:07:44.896877Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 692,
"name": "MODELMAG_U",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.728362Z",
"updated": "2021-02-09T04:07:44.908824Z",
"contact": null,
"ucd": "phot.mag;em.opt.U",
"unit": "mag"
},
{
"id": 693,
"name": "MODELMAG_Z",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.763787Z",
"updated": "2021-02-09T04:07:44.920782Z",
"contact": null,
"ucd": "phot.mag;em.opt",
"unit": "mag"
},
{
"id": 694,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS objid",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.806981Z",
"updated": "2021-02-09T04:07:44.932808Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 695,
"name": "PETROMAG_G",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.851467Z",
"updated": "2021-02-09T04:07:44.943949Z",
"contact": null,
"ucd": "phot.mag;em.opt",
"unit": "mag"
},
{
"id": 696,
"name": "PETROMAG_I",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.889072Z",
"updated": "2021-02-09T04:07:44.955412Z",
"contact": null,
"ucd": "phot.mag;em.opt.I",
"unit": "mag"
},
{
"id": 697,
"name": "PETROMAG_R",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.917162Z",
"updated": "2021-02-09T04:07:44.967299Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 698,
"name": "PETROMAG_U",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.935105Z",
"updated": "2021-02-09T04:07:44.979016Z",
"contact": null,
"ucd": "phot.mag;em.opt.U",
"unit": "mag"
},
{
"id": 699,
"name": "PETROMAG_Z",
"pretty_name": null,
"description": "DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.969980Z",
"updated": "2021-02-09T04:07:44.990853Z",
"contact": null,
"ucd": "phot.mag;em.opt",
"unit": "mag"
},
{
"id": 700,
"name": "PETROR50_R",
"pretty_name": null,
"description": "Radius containing 50% of Petrosian flux",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:12.988706Z",
"updated": "2021-02-09T04:07:45.002992Z",
"contact": null,
"ucd": "phys.angSize;em.opt.R",
"unit": "arcsec"
},
{
"id": 701,
"name": "PETROR90_R",
"pretty_name": null,
"description": "Radius containing 90% of Petrosian flux",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.008238Z",
"updated": "2021-02-09T04:07:45.015751Z",
"contact": null,
"ucd": "phys.angSize;em.opt.R",
"unit": "arcsec"
},
{
"id": 702,
"name": "PETRORAD_R",
"pretty_name": null,
"description": "Petrosian radius",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.027844Z",
"updated": "2021-02-09T04:07:45.027749Z",
"contact": null,
"ucd": "phys.angSize;em.opt.R",
"unit": "arcsec"
},
{
"id": 703,
"name": "PRIMTARGET",
"pretty_name": null,
"description": "See SDSS photoobj table",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.055002Z",
"updated": "2021-02-09T04:07:45.040013Z",
"contact": null,
"ucd": "meta.code.class",
"unit": "-"
},
{
"id": 704,
"name": "PSFMAG_R",
"pretty_name": null,
"description": "PSF magnitude",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.082347Z",
"updated": "2021-02-09T04:07:45.052202Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 705,
"name": "RA",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.103297Z",
"updated": "2021-02-09T04:07:45.065159Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 706,
"name": "RUN",
"pretty_name": null,
"description": "SDSS run number",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.123191Z",
"updated": "2021-02-09T04:07:45.076920Z",
"contact": null,
"ucd": "obs.param",
"unit": "-"
},
{
"id": 707,
"name": "STATUS",
"pretty_name": null,
"description": "See SDSS photoobj table",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.142270Z",
"updated": "2021-02-09T04:07:45.090941Z",
"contact": null,
"ucd": "meta.code.status",
"unit": "-"
}
]
},
{
"id": 27,
"name": "TilingCat",
"pretty_name": null,
"description": "Science targets and information for tiling and spectroscopic observation.",
"documentation": "InputCat<br>TilingCat<br>v16<br>2011-07-21<br>Ivan Baldry <ikb@astro.livjm.ac.uk><br><br>This catalog is used to keep track of the state of the survey. During<br>survey operations it is updated as soon as new redshifts are available<br>and it is used to set the priorities for the next observing run. The<br>present version of this catalog is the final GAMA I version (i.e.<br>after the completion of all GAMA I observations).<br><br>Note that this table contains the complete tiling catalog, not just<br>the objects for which redshifts are released in DR2 (r < 19.0 in G09<br>and G12, and r < 19.4 in G15). Objects included in DR2 may be<br>identified using the column DR2_FLAG. Those objects for which<br>redshifts are not released in DR2 have their redshift column Z set to<br>-9.99999. However, the redshift quality column NQ has not been<br>modified, and so this column informs users whether a good quality<br>redshift for this object exists (but is not released yet).<br><br>This table is derived from InputCatA, selecting GAMA regions (12x4<br>deg^2; G09, G12, G15), applying magnitude limits, star-galaxy<br>separation, surface-brightness limits, and mask.<br><br>The full details are given in the Input Catalog (IC) paper, <a href=\"http://adsabs.harvard.edu/abs/2010MNRAS.404...86B\">Baldry et<br>al. (2010)</a>.<br><br>The redshifts in this table are obtained from table SpecAll in the<br>SpecCat DMU by matching by CATAID except for a few cases. There are 5<br>cases where an object is matched within 1 arcsec to a spectrum that<br>has been assigned to another object.<br><br>In the following we provide some additional information on individual<br>columns of this table.<br><br>...............................................................................<br><br>SURVEY_CODE for source of redshift<br><br>1=SDSS, 2=2dFGRS, 3=MGC, 4=2SLAQ-LRG, 5=GAMA, 6=6dFGS, 7=UZC, 8=2QZ,<br>9=2SLAQ-QSO, 10=NED, 11=GAMA_LT, 12=WiggleZ<br>...............................................................................<br><br>TARGET_FLAGS (t) (showing which target criteria are satisfied)<br>(bitwise set of flags, bit X): <br><br>X t=2^X meaning<br>0 1 SDSS main galaxy sample<br>1 2 SDSS LRG sample<br>2 4 r < 19.0 and r_psf-r_model > 0.25 (high priority in Year 1)<br>3 8 r < 19.4 (G09,G15) or r < 19.8 (G12)<br>4 16 r < 19.8<br>5 32 z_model < 18.2<br>6 64 K_AB < 17.6<br>7 128 (g_model < 20.6 or r_model < 19.8 or i_model < 19.4) (G12)<br>8 256 radio_flux > 0.0<br>...............................................................................<br><br>SURVEY_CLASS (sc)<br><br>sc = 0: not a target (except for checks on vis_class=3)<br>sc = 1: target only because of radio selection (F1 not (MS or F2 or F3))<br>sc >= 2: passes star-galaxy separation criteria (MS, F2 or F3)<br>sc >= 3: r < 19.8 or zK-selected (MS, F2) (uniform selection in all regions)<br>sc >= 4: *** MS ***<br>sc >= 5: MS r or z-selected <br>sc >= 6: *** MS r-selected only ***<br>sc >= 7: r < 19.0 and sg_sep > 0.25 (Year 1 high priority targets)<br><br>See the IC paper for details on the selection. 'MS' means main survey:<br>main survey = <br>(r < 19.4 (G09,G15) or r < 19.8 (G12) or K_AB < 17.6 or z_{model} < 18.2)<br><br>For science catalogs: select, for example, <br>SURVEY_CLASS >= 4 for all main survey targets (see IC paper), <br>SURVEY_CLASS >= 6 for r-selection only (r < 19.4 in G09 & G15, r < 19.8 in G12)<br><br>F1, F2, and F3 are filler selections. These targets are only allocated<br>a fibre when the fibre cannot be allocated to a MS target.<br><br>DR2 only includes data for MS objects, i.e. SURVEY_CLASS >= 4.<br><br>Further note: Objects with target_flags=0 (also survey_class=0) have<br>2<=vis_class<=4 or they are excluded by Eq. 12 only of the IC paper<br>(Sec. 5.2). These remain in the tiling catalogue because they are rejected by<br>a more subjective criteria than the other selections.<br>...............................................................................<br><br>MASK_IC_10 / MASK_IC_12:<br><br>These parameters encode the bright star mask. The bright star mask is<br>based on stars in the Tycho 2, Tycho 1 and Hipparcos catalogues. For<br>each bright star, a scattered-light radius (R_s) was estimated based<br>on the circular region over which the star flux per pixel is greater<br>than five times the sky noise level. For each object in TilingCat<br>MASK_IC_10 is defined as follows:<br><br> d <= R_s : MASK_IC_10 = 1<br>R_s < d <= 5*R_s : MASK_IC_10 = R_s / d<br> d > 5*R_s : MASK_IC_10 = 0<br><br>where d is the distance between the object and the nearest V < 10 mag<br>star, which has scattered light radius R_s. In other words, the<br>MASK_IC_10 value decreases from unity when d <= R_s to 0.2 when d =<br>5*R_s, and then jumps to 0 when d > 5*R_s. MASK_IC_12 is defined in<br>the same way for V < 12 mag stars. In addition, objects within an SDSS<br>database mask for holes, satellite trails or bleeding pixels had these<br>mask values set to unity.<br>...............................................................................<br><br>PRIORITY_CLASS (p):<br><br>p > 1 except p=2,4,7 satisfy survey_class >= 3; <br>p > 1 satisfy fiber mag limits 16.8 < r_fib < 22.8;<br>p > 1 expect p=7 satisfy vis_class<=1 or vis_class=255. <br><br>p=9: Q<=2 and num_gama_spec = 0 (target but never attempted)<br>p=8: Q<=2 and num_gama_spec = 1 (only one failed GAMA observation)<br><br>p=7: Q<=2 and vis_class=3 (would be a target other than vis_class)<br>p=6: Q=3 and num_gama_spec <=1 (to check the Q=3 redshift blunder rate)<br><br>p=5: Q<=2 and num_gama_spec >=2 (two or more failed GAMA observations)<br>p=4: Q<=2 other targets (sc=1 or sc=2)<br><br>p=3: Q=3 and num_gama_spec >=2 or Q >= 4 (sc >= 3 done)<br>p=2: Q >= 3 other targets (sc=1 or sc=2 done)<br><br>p=0: all others including: vis_class=2-4 objects, fibre bright or fibre faint. <br>...............................................................................<br><br>VIS_CLASS for visual classification<br><br>0 = not eyeballed<br>1 = yes a target<br>2 = not a target (no evidence of galaxy light)<br>3 = not a target (not the main part of a galaxy)<br>4 = compromised photometry (selection mag has serious error)<br>255 = not eyeballed but the following flags are *all* zero<br> EDGE, BLENDED, CHILD, MAYBE_CR, MAYBE_EGHOST<br>...............................................................................<br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/TilingCat.fits",
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"type": "CatalogueTable",
"created": "2021-01-28T00:39:53.971040Z",
"updated": "2021-02-09T04:08:05.822376Z",
"contact": {
"email": "ikb@astro.livjm.ac.uk",
"name": "Ivan Baldry "
},
"input_cat": true,
"columns": [
{
"id": 720,
"name": "CATAID",
"pretty_name": null,
"description": "Unique GAMA ID of object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.679393Z",
"updated": "2021-02-09T04:07:45.253621Z",
"contact": null,
"ucd": "meta.id;meta.main",
"unit": "-"
},
{
"id": 721,
"name": "DEC",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.707233Z",
"updated": "2021-02-09T04:07:45.277909Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 722,
"name": "DR2_FLAG",
"pretty_name": null,
"description": "Indicates whether spectra, redshifts and ancillary data for this object are released in DR2",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.742179Z",
"updated": "2021-02-09T04:07:45.289880Z",
"contact": null,
"ucd": "meta.code",
"unit": "-"
},
{
"id": 723,
"name": "FIBERMAG_R",
"pretty_name": null,
"description": "3-arcsec fiber magnitude",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.769898Z",
"updated": "2021-02-09T04:07:45.301655Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 724,
"name": "G_MODEL",
"pretty_name": null,
"description": "Extinction-corrected SDSS DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.808651Z",
"updated": "2021-02-09T04:07:45.313474Z",
"contact": null,
"ucd": "phot.mag;em.opt.B",
"unit": "mag"
},
{
"id": 725,
"name": "I_MODEL",
"pretty_name": null,
"description": "Extinction-corrected SDSS DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.844845Z",
"updated": "2021-02-09T04:07:45.325215Z",
"contact": null,
"ucd": "phot.mag;em.opt.I",
"unit": "mag"
},
{
"id": 726,
"name": "K_AUTO",
"pretty_name": null,
"description": "Extinction-corrected r-defined auto AB mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.884064Z",
"updated": "2021-02-09T04:07:45.336976Z",
"contact": null,
"ucd": "phot.mag;em.IR.K",
"unit": "mag"
},
{
"id": 727,
"name": "MASK_IC_10",
"pretty_name": null,
"description": "Mask value 0.0 to 1.0 around V<10 stars",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.910405Z",
"updated": "2021-02-09T04:07:45.348354Z",
"contact": null,
"ucd": "meta.code",
"unit": "-"
},
{
"id": 728,
"name": "MASK_IC_12",
"pretty_name": null,
"description": "Mask value 0.0 to 1.0 around V<12 stars",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.942619Z",
"updated": "2021-02-09T04:07:45.365953Z",
"contact": null,
"ucd": "meta.code",
"unit": "-"
},
{
"id": 729,
"name": "NEIGHBOUR_CLASS",
"pretty_name": null,
"description": "Number of priority_class>=8 targets within 40 arcsec",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:13.975351Z",
"updated": "2021-02-09T04:07:45.377761Z",
"contact": null,
"ucd": "meta.code.class",
"unit": "-"
},
{
"id": 730,
"name": "NQ",
"pretty_name": null,
"description": "Quality of redshift",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.001408Z",
"updated": "2021-02-09T04:07:45.388973Z",
"contact": null,
"ucd": "meta.code.qual;src.redshift",
"unit": "-"
},
{
"id": 731,
"name": "NUM_GAMA_SPEC",
"pretty_name": null,
"description": "Number of GAMA spectra matched to object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.037056Z",
"updated": "2021-02-09T04:07:45.400431Z",
"contact": null,
"ucd": "meta.number;spect",
"unit": "-"
},
{
"id": 732,
"name": "OBJID",
"pretty_name": null,
"description": "SDSS objid",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.080871Z",
"updated": "2021-02-09T04:07:45.419687Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 733,
"name": "PRIORITY_CLASS",
"pretty_name": null,
"description": "Priorities for targeting, see notes",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.123506Z",
"updated": "2021-02-09T04:07:45.434023Z",
"contact": null,
"ucd": "meta.code.class",
"unit": "-"
},
{
"id": 734,
"name": "RA",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.158885Z",
"updated": "2021-02-09T04:07:45.447463Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 735,
"name": "R_MODEL",
"pretty_name": null,
"description": "Extinction-corrected SDSS DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.210595Z",
"updated": "2021-02-09T04:07:45.460254Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 736,
"name": "R_PETRO",
"pretty_name": null,
"description": "Extinction-corrected SDSS DR6 Petrosian mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.246230Z",
"updated": "2021-02-09T04:07:45.490259Z",
"contact": null,
"ucd": "phot.mag;em.opt.R",
"unit": "mag"
},
{
"id": 737,
"name": "R_SB",
"pretty_name": null,
"description": "SDSS Petro half-light surface brightness",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.264664Z",
"updated": "2021-02-09T04:07:45.511611Z",
"contact": null,
"ucd": "phot.mag.sb;em.opt.R",
"unit": "mag/arcsec^2"
},
{
"id": 738,
"name": "SG_SEP",
"pretty_name": null,
"description": "r_psf - r_model star-galaxy separation parameter",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.304451Z",
"updated": "2021-02-09T04:07:45.533578Z",
"contact": null,
"ucd": "src.class.starGalaxy",
"unit": "mag"
},
{
"id": 739,
"name": "SG_SEP_JK",
"pretty_name": null,
"description": "J - K - f_locus star-galaxy separation parameter",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.323449Z",
"updated": "2021-02-09T04:07:45.562529Z",
"contact": null,
"ucd": "src.class.starGalaxy",
"unit": "mag"
},
{
"id": 740,
"name": "SPECID",
"pretty_name": null,
"description": "ID of spectrum from SpecAll table",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.349291Z",
"updated": "2021-02-09T04:07:45.575145Z",
"contact": null,
"ucd": "meta.id.cross;spect",
"unit": "-"
},
{
"id": 741,
"name": "SURVEY_CLASS",
"pretty_name": null,
"description": "Useful for selecting samples, see notes",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.370822Z",
"updated": "2021-02-09T04:07:45.587575Z",
"contact": null,
"ucd": "meta.code.class",
"unit": "-"
},
{
"id": 742,
"name": "SURVEY_CODE",
"pretty_name": null,
"description": "Survey code for redshift source, see notes",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.406750Z",
"updated": "2021-02-09T04:07:45.599712Z",
"contact": null,
"ucd": "meta.code;meta.dataset",
"unit": "-"
},
{
"id": 743,
"name": "TARGET_FLAGS",
"pretty_name": null,
"description": "Bitwise target criteria, see notes",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.442024Z",
"updated": "2021-02-09T04:07:45.611940Z",
"contact": null,
"ucd": "meta.code",
"unit": "-"
},
{
"id": 744,
"name": "U_MODEL",
"pretty_name": null,
"description": "Extinction-corrected SDSS DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.462482Z",
"updated": "2021-02-09T04:07:45.623787Z",
"contact": null,
"ucd": "phot.mag;em.opt.U",
"unit": "mag"
},
{
"id": 745,
"name": "VIS_CLASS",
"pretty_name": null,
"description": "Visual classification, see notes",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.484632Z",
"updated": "2021-02-09T04:07:45.635874Z",
"contact": null,
"ucd": "mata.code.qual",
"unit": "-"
},
{
"id": 746,
"name": "VIS_CLASS_USER",
"pretty_name": null,
"description": "Initials of classifiers, xxx for none",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.530501Z",
"updated": "2021-02-09T04:07:45.649955Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 747,
"name": "Z",
"pretty_name": null,
"description": "Spectroscopic redshift, -1 for none attempted",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.563049Z",
"updated": "2021-02-09T04:07:45.662383Z",
"contact": null,
"ucd": "src.redshift",
"unit": "-"
},
{
"id": 748,
"name": "Z_MODEL",
"pretty_name": null,
"description": "Extinction-corrected SDSS DR6 mag",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.586397Z",
"updated": "2021-02-09T04:07:45.676270Z",
"contact": null,
"ucd": "phot.mag;em.opt.I",
"unit": "mag"
}
]
}
]
},
{
"id": 10,
"name": "LocalFlowCorrection",
"pretty_name": "LocalFlowCorrection",
"description": "This DMU performs local flow correction, and provides redshifts in different frames of reference.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v07",
"type": "CatalogueGroup",
"created": "2021-01-28T00:39:53.080316Z",
"updated": "2021-02-09T04:07:34.495721Z",
"contact": {
"email": "ikb@astro.livjm.ac.uk",
"name": "Ivan Baldry "
},
"tables": [
{
"id": 28,
"name": "DistancesFrames",
"pretty_name": null,
"description": "This table provides redhifts in various reference frames, flow corrected redshifts, and distance moduli for all GAMA DR2 objects.",
"documentation": "LocalFlowCorrection<br>DistancesFrames<br>v07<br>2011-11-22<br>Ivan Baldry <ikb@astro.livjm.ac.uk><br><br>This table provides redshifts in various reference frames, flow<br>corrected redshifts, and distance moduli for all GAMA DR2 objects with<br>z > -0.01 and nQ >= 2. Note that only nQ >= 3 redshifts should be<br>considered reliable.<br><br>The implementation of the frame and flow-model redshifts is described<br>in section 2.3 of <a href=\"http://adsabs.harvard.edu/abs/2012MNRAS.421..621B\">Baldry et al. (2012)</a>. The effect on the distance<br>moduli is significant at z < 0.03, see figure 2 of the paper.<br><br>The heliocentric redshifts are obtained from the table <a href=\"/dr2/schema/table.php?name=SpecAll\">SpecAll</a> in the<br><a href=\"/dr2/schema/dmu.php?name=SpecCat\">SpecCat DMU</a>.<br><br>CMB frame uses the dipole from <a href=\"http://adsabs.harvard.edu/abs/1996ApJ...470...38L\">Lineweaver et al. (1996)</a>; and the Local<br>Group frame uses the conversion from <a href=\"http://adsabs.harvard.edu/abs/1999AJ....118..337C\">Courteau & van den Bergh (1999)</a>.<br><br>z_tonry uses the <a href=\"http://adsabs.harvard.edu/abs/2000ApJ...530..625T\">Tonry et al. (2000)</a> flow model described in the<br>Appendix of that paper. Note there are triple-valued solutions of<br>z_cmb -> z_tonry over a small range in G12 (near Virgo cluster), here<br>the average distance is used. The solution is tapered to z_cmb from<br>z_cmb = 0.02 to z_cmb = 0.03. Thus z_tonry = z_cmb at z_cmb > 0.03.<br>z_tonry is close to but not exactly equal to z_lg (Local Group frame<br>redshift) at < ~10 Mpc.<br><br>The distance moduli given in the table are determined using z_tonry<br>only for entries where the velocity (c z_tonry) > 300 km/s (z > 0.001;<br>D_L > 3 Mpc/h). Note this does not guarantee that stars with large<br>redshift errors will be excluded. Either the spectra and images need<br>to be checked or a more restrictive cut should be used. For objects<br>with z < 0.001, the distance modulus is not calculated and is given<br>the value zero.<br><br>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/DistancesFrames.fits",
"file_name": "DistancesFrames.fits",
"file_extension": "fits",
"version": "v07",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:54.006744Z",
"updated": "2021-02-09T04:07:35.001727Z",
"contact": {
"email": "ikb@astro.livjm.ac.uk",
"name": "Ivan Baldry "
},
"input_cat": false,
"columns": [
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"id": 749,
"name": "CATAID",
"pretty_name": null,
"description": "Unique ID of GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.627332Z",
"updated": "2021-02-09T04:07:45.690084Z",
"contact": null,
"ucd": "meta.id;meta.main",
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},
{
"id": 750,
"name": "DEC",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
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"created": "2021-01-28T00:40:14.659688Z",
"updated": "2021-02-09T04:07:45.702013Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 751,
"name": "DM_100_25_75",
"pretty_name": null,
"description": "distance modulus for H0=100, 0.25, 0.75",
"documentation": "",
"file_path": null,
"file_name": null,
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:14.693074Z",
"updated": "2021-02-09T04:07:45.715626Z",
"contact": null,
"ucd": "phot.mag.distMod",
"unit": "mag"
},
{
"id": 752,
"name": "DM_100_30_70",
"pretty_name": null,
"description": "distance modulus for H0=100, 0.30, 0.70",
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"created": "2021-01-28T00:40:14.720260Z",
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{
"id": 753,
"name": "DM_70_30_70",
"pretty_name": null,
"description": "distance modulus for 737 cosmology",
"documentation": "",
"file_path": null,
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"created": "2021-01-28T00:40:14.763451Z",
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},
{
"id": 754,
"name": "NQ",
"pretty_name": null,
"description": "quality of redshift (use nQ > 2 for science)",
"documentation": "",
"file_path": null,
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"file_extension": null,
"version": null,
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"created": "2021-01-28T00:40:14.791502Z",
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"name": "RA",
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"description": "J2000 coordinate",
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"created": "2021-01-28T00:40:14.819319Z",
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{
"id": 756,
"name": "Z_CMB",
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"description": "CMB frame redshift",
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"created": "2021-01-28T00:40:14.854755Z",
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"name": "Z_HELIO",
"pretty_name": null,
"description": "heliocentric redshift",
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"created": "2021-01-28T00:40:14.889239Z",
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"name": "Z_LG",
"pretty_name": null,
"description": "Local Group frame redshift",
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{
"id": 759,
"name": "Z_TONRY",
"pretty_name": null,
"description": "flow corrected redshift using Tonry et al. model",
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"created": "2021-01-28T00:40:14.945267Z",
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"description": "recomputed after adjusting z_helio by +180 km/s",
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{
"id": 11,
"name": "SersicPhotometry",
"pretty_name": "SersicPhotometry",
"description": "This DMU provides a single-component Sersic fit in each of the ugrizYJHK bands for every GAMA DR2 galaxy.",
"documentation": "SersicPhotometry<br>2011-10-13<br>Lee Kelvin <lee.kelvin@uibk.ac.at><br><br>The SersicPhotometry DMU produces a single-Sersic (1-component only)<br>fit to every GAMA DR2 object in each of the bands ugrizYJHK. This is<br>achieved by using SIGMA v0.9-0 (Structural Investigation of Galaxies<br>via Model Analysis) on SDSS and UKIDSS LAS imaging data. SIGMA is a<br>wrapper around several contemporary astronomy tools such as Source<br>Extractor (<a href=\"http://adsabs.harvard.edu/abs/1996A%26AS..117..393B\">Bertin & Arnouts 1996</a>), PSF Extractor (Bertin and Delorme,<br>priv. comm.) and GALFIT 3 (<a href=\"http://adsabs.harvard.edu/abs/2010AJ....139.2097P\">Peng et al. 2010</a>), as well as analysis and<br>processing code writting in the open-source <a href=\"http://www.r-project.org/\">R programming language</a> (R<br>Development Core Team, 2010). Please cite <a href=\"http://adsabs.harvard.edu/abs/2012MNRAS.421.1007K\">Kelvin et al. (2012)</a> when<br>using data products from this DMU.<br><br>GALFIT is the workhorse fitting algorithm used within SIGMA. To<br>produce a model of a galaxy, GALFIT must be provided with suitable<br>starting parameters (such as size, magnitude, ellipticity, etc), an<br>appropriate PSF and cutouts of both the science data and any<br>associated weight maps. The cutouts are created from the GAMA v02<br>mosaics (available on the <a/ href=\"/dr2/data/imaging/gama/mosaics/v02/\">DR2 file server</a>, swpim* files), with<br>physical initial conditions and the PSF provided by Source Extractor<br>and PSF Extractor, respectively. These programs are called and setup<br>automatically within the SIGMA script, their outputs reprocessed into<br>a form GALFIT is able to read, and fed into GALFIT. GALFIT uses a<br>simple downhill minimisation in order to minimise the global-chi^2 of<br>the model. Its outputs are analysed by SIGMA for any obvious errors,<br>and if found, an attempt at fixing them will automatically be made.<br><br>This DMU provides two tables: SersicCatAll and SersicCat. The former<br>contains a complete record of all of the outputs produced by<br>SIGMA. The latter table only contains those columns considered to be<br>most useful to the users. In other words, SersicCat contains an exact<br>subset of the columns in SersicCatAll.<br><br>Below are more detailed notes on several of the columns provided by<br>the SersicPhotometry DMU. The unique identifier for the<br>SersicPhotometry DMU is the CATAID (column 1) which refers to the GAMA<br>ID of an object. Null entries in SersicCat are labelled -9999. For<br>further details on the operation of SIGMA, please refer to Kelvin et<br>al. (2012).<br><br>##############################################################################<br><br>Dependencies:<br> InputCat TilingCat<br> Mosaics v02<br><br>##############################################################################<br><br>Potential zero-point offsets<br><br>Please see the notes of the table <a href=\"/dr2/schema/table.php?name=ApMatchedCat\">ApMatchedCat</a>.<br><br>##############################################################################<br><br>SIGMA_INDEX<br><br>A unique identifier that the SIGMA code uses to identify each<br>galaxy. This remains a part of SIGMA for historical reasons.<br><br>##############################################################################<br><br>OBJNAME<br><br>SIGMA_INDEX, padded with leading zeroes to make the total length 8<br>characters long, and then prefixed with an S to construct the OBJNAME.<br>This name is more commonly used when saving modelling data within the<br>GAMA database.<br><br>##############################################################################<br><br>URL<br><br>Location of the directory on the <a href=\"/dr2/data/\">file server</a> containing all of the<br>input and output files used and produced by SIGMA for this galaxy. For<br>more details on the contents of this directory see the directory<br>description on the file server.<br><br>Please note that the world coordinate system (WCS) information in the<br>headers of the various fits files found in this directory is partially<br>incorrect. The pixel sizes are correct, but the absolute positions<br>implied by the WCS information in the header are incorrect.<br><br>##############################################################################<br><br>PSF_<br><br>All columns starting with 'PSF_' are outputs of the PSF Extractor<br>pipeline within SIGMA. These outputs are provided for reference only<br>to aid in the understanding of the final single-Sersic model. For more<br>information, see Kelvin et al. (2012).<br><br>##############################################################################<br><br>SEX_<br><br>All columns starting with 'SEX_' are outputs of the Source Extractor<br>pipeline within SIGMA. These Source Extractor outputs provided the<br>starting parameters for the GALFIT inputs used during minimisation.<br>These outputs are provided *for reference only* to aid in the<br>understanding of the final single-Sersic model. Unless there is a very<br>good reason to do so, these should not be used in scientific analyses.<br>Their GAL_ equivalents (see below) should be used instead. For more<br>information, see Kelvin et al. (2012).<br><br>##############################################################################<br><br>GAL_<br><br>All columns starting with 'GAL_' are final outputs of the GALFIT<br>pipeline within SIGMA. These GALFIT outputs provide the main output of<br>the SersicPhotometry DMU. For more information, see Kelvin et al. (2012).<br><br>##############################################################################<br><br>SEX_PA/GAL_PA<br><br>The position angle on the image recovered from Source Extractor and<br>GALFIT, respectively. This is defined from the positive x-axis of the<br>image (roughly aligned to west), increasing from zero anti-clockwise.<br><br>NOTE: SEX_PA goes from -90 to +90, whereas GAL_PA goes from 0 to +180,<br>however the definitions below still hold true at all times.<br><br>x-positive 0 degrees<br>y-positive 90 degrees<br>x-negative 180 degrees (equivalent to x-positive, redundant)<br>y-negative -90 degrees (equivalent to y-positive, redundant)<br><br>Unfortunately, due to an oversight, this DMU does *not* include<br>equivalent angles on the sky. However, an approximate on-sky angle can<br>be recovered as<br><br>SEX_PA_J2000_X = SEX_PA_X + (THETA_J2000 - THETA_IMAGE)<br>GAL_PA_J2000_X = GAL_PA_X + (THETA_J2000 - THETA_IMAGE)<br><br>where THETA_J2000 and THETA_IMAGE are the on-sky and on-image position<br>angles, respectively, listed in the table ApMatchedCat in the<br>ApMatchedPhotom DMU.<br><br>Despite this being only an approximation we recommend the use of<br>GAL_PA_J2000_X over THETA_J2000.<br><br>Note that SEX_PA_R in this DMU and THETA_IMAGE in the ApMatchedPhotom<br>DMU are not identical due to the procedures employed by these DMUs<br>being slightly different.<br><br>##############################################################################<br><br>GAL_FIT<br><br>The function combination chosen to model. Since the SersicPhotometry<br>is tasked with fitting a single-Sersic component to every galaxy, this<br>value will always be either 1 or -9999 (null). GAL_FITWORD gives the<br>corresponding word describing the combination chosen to model instead<br>of a number.<br><br>1 Sersic<br>2 Sersic + Exponential<br>3 Sersic + Sersic disk<br>4 Sersic bulge + Sersic disk (bulge/disk Re < 1, bulge/disk n > 1)<br>5 de Vaucouleurs + Exponential<br>-9999 Null<br><br>##############################################################################<br><br>GAL_RESULT<br><br>The end result of the GALFIT fitting stage. <br><br>CRASH An error has occurred causing the code to crash, usually due to bad <br> inputs caused by nearby star contamination or bad data.<br><br>ERROR A fatal error has occurred within GALFIT causing the code to <br> quit before minimisation. Usually caused by extremely bad inputs from <br> Source Extractor, or a bad PSF.<br><br>OKAY GALFIT completed successfully and SIGMA was happy enough with its<br> outputs to move on to the next galaxy in the catalogue. A flag<br> of OKAY does not mean that the result is perfect, i.e. physically <br> meaningful, it merely reflects that GALFIT was able to finish <br> without a major error occurring.<br><br>##############################################################################<br><br>GAL_QFLAG<br><br>This is a binary flag, and describes the quality of the final fit. <br>Flags may add together to produce a number higher than 1024.<br><br>0 fine<br>1 no object detected<br>2 compromised photometry (an object brighter than 0.75 mags fainter than<br> the primary lies within 4re)<br>4 magnitude between SEx and GALFIT differs by +-1 mag<br>8 crash/error<br>16 center migrated (> 5 pixels)<br>32 max. iterations (100)<br>64 large radius (ln[RAD/FLUXRAD]>2)<br>128 small radius (ln[RAD/FLUXRAD]<-2)<br>256 high Sersic index (n>10)<br>512 high ellipticity (e>0.95)<br>1024 bad chi2 (chi2<0.5 or chi2>2)<br><br>##############################################################################<br><br>GAL_GHFLAG<br><br>This is a binary flag, and describes the global fitting history<br>(i.e. non-Sersic specific).<br><br>Flags may add together to produce a number higher than 4. Multiple<br>runs cause the GHFLAG value to loop over and start at the next logical<br>binary operator (1,2,4,8,16,32...), and so many fitting runs can cause<br>GHFLAG to get very large. Example: the first run has a bad chi2 and<br>reached its maximum iterations, whereas the second run only had a bad<br>chi2. This would give 4+2 from run 1, and 32 from run 2, giving a<br>total GHFLAG of 38.<br><br>0 fine<br>1 crash/error<br>2 max iterations (100)<br>4 bad chi2 (chi2<0.5 or chi2>2)<br><br>##############################################################################<br><br>GAL_CHFLAG<br><br>This is a binary flag, and describes the component fitting history<br>(i.e. Ssersic specific).<br><br>Flags may add together to produce a number higher than 16. Multiple<br>runs cause the CHFLAG value to loop over and start at the next logical<br>binary operator (1,2,4,8,16,32...), and so many fitting runs can cause<br>CHFLAG to get very large. Example: the first run has a high<br>ellipticity and a high Sersic index, and the second run has a large<br>radius. This would give 16+8 from run 1, and 64 from run 2, giving a<br>total CHFLAG of 88.<br><br>0 fine<br>1 center migrated (> SEx re)<br>2 large radius (ln[RAD/FLUXRAD]>3)<br>4 small radius (ln[RAD/FLUXRAD]<-3)<br>8 high Sersic index (n>10)<br>16 high ellipticity (e>0.95)<br><br>##############################################################################<br><br>GAL_TYPE<br><br>GALFIT output type. Since the SersicPhotometry DMU is tasked with<br>fitting a single-Sersic component to every galaxy, this value will<br>always be either 1, 2, 5 or -9999 (null). GAL_TYPEWORD gives the<br>corresponding word describing the output type instead of a number.<br><br>1 crash<br>2 error<br>3 sky<br>4 psf<br>5 sersic<br>6 expdisk<br>7 edgedisk<br>8 ferrer<br>9 nuker<br>-9999 Null<br><br>##############################################################################<br><br>_MAG_<br><br>Magnitudes presented in this catalogue have not been corrected for the<br>effect of foreground Milky Way dust extinction. Should these<br>corrections be required, they can be obtained from the table<br>GalacticExtinction in the InputCat DMU.<br><br>All photometry is on the AB system.<br><br>##############################################################################<br><br>",
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"created": "2021-01-28T00:39:53.104583Z",
"updated": "2021-02-09T04:07:34.506099Z",
"contact": {
"email": "lee.kelvin@uibk.ac.at",
"name": "Lee Kelvin "
},
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"contact": {
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"name": "GAL_DEC_H",
"pretty_name": null,
"description": "Declination as determined by GALFIT",
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"id": 909,
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"description": "SIGMA Object name (see notes)",
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"contact": null,
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},
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"id": 764,
"name": "FILENAME",
"pretty_name": null,
"description": "Full path to object`s data directory",
"documentation": "",
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"created": "2021-01-28T00:40:15.077160Z",
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"description": "reduced Chi^2 of output model",
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"created": "2021-01-28T00:40:15.110516Z",
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"description": "reduced Chi^2 of output model",
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"created": "2021-01-28T00:40:15.134653Z",
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"id": 767,
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"pretty_name": null,
"description": "reduced Chi^2 of output model",
"documentation": "",
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"id": 768,
"name": "GAL_CHI2_J",
"pretty_name": null,
"description": "reduced Chi^2 of output model",
"documentation": "",
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"version": null,
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"created": "2021-01-28T00:40:15.194177Z",
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"contact": null,
"ucd": "stat.fit.goodness;em.opt.U",
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{
"id": 1268,
"name": "PSF_CHI2_Y",
"pretty_name": null,
"description": "PSFEx PSF reduced Chi^2",
"documentation": "",
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"created": "2021-01-28T00:40:31.099526Z",
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"pretty_name": null,
"description": "PSFEx PSF reduced Chi^2",
"documentation": "",
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"created": "2021-01-28T00:40:31.139923Z",
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"id": 1270,
"name": "PSF_FWHM_G",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
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"created": "2021-01-28T00:40:31.174297Z",
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"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.opt",
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},
{
"id": 1271,
"name": "PSF_FWHM_H",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.191590Z",
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"ucd": "instr.det.psf;meta.modelled;em.IR.H",
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},
{
"id": 1272,
"name": "PSF_FWHM_I",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.208672Z",
"updated": "2021-02-09T04:07:53.367931Z",
"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.opt.I",
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},
{
"id": 1273,
"name": "PSF_FWHM_J",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.226330Z",
"updated": "2021-02-09T04:07:53.398667Z",
"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.IR.J",
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},
{
"id": 1274,
"name": "PSF_FWHM_K",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.244946Z",
"updated": "2021-02-09T04:07:53.421128Z",
"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.IR.K",
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},
{
"id": 1275,
"name": "PSF_FWHM_R",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.264130Z",
"updated": "2021-02-09T04:07:53.450933Z",
"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.opt.R",
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},
{
"id": 1276,
"name": "PSF_FWHM_U",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.283327Z",
"updated": "2021-02-09T04:07:53.481917Z",
"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.opt.U",
"unit": "arcsec"
},
{
"id": 1277,
"name": "PSF_FWHM_Y",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.302787Z",
"updated": "2021-02-09T04:07:53.503920Z",
"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.IR.NIR",
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},
{
"id": 1278,
"name": "PSF_FWHM_Z",
"pretty_name": null,
"description": "PSFEx PSF FWHM",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.331213Z",
"updated": "2021-02-09T04:07:53.533805Z",
"contact": null,
"ucd": "instr.det.psf;meta.modelled;em.opt",
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},
{
"id": 1279,
"name": "PSF_NUM_G",
"pretty_name": null,
"description": "PSFEx number of stars used",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.349289Z",
"updated": "2021-02-09T04:07:53.564797Z",
"contact": null,
"ucd": "meta.number;em.opt",
"unit": "-"
},
{
"id": 1280,
"name": "PSF_NUM_H",
"pretty_name": null,
"description": "PSFEx number of stars used",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.369271Z",
"updated": "2021-02-09T04:07:53.581002Z",
"contact": null,
"ucd": "meta.number;em.IR.H",
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},
{
"id": 1281,
"name": "PSF_NUM_I",
"pretty_name": null,
"description": "PSFEx number of stars used",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.387876Z",
"updated": "2021-02-09T04:07:53.610629Z",
"contact": null,
"ucd": "meta.number;em.opt.I",
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},
{
"id": 1282,
"name": "PSF_NUM_J",
"pretty_name": null,
"description": "PSFEx number of stars used",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.407840Z",
"updated": "2021-02-09T04:07:53.632540Z",
"contact": null,
"ucd": "meta.number;em.IR.J",
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},
{
"id": 1283,
"name": "PSF_NUM_K",
"pretty_name": null,
"description": "PSFEx number of stars used",
"documentation": "",
"file_path": null,
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"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.428815Z",
"updated": "2021-02-09T04:07:53.661871Z",
"contact": null,
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},
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"id": 1284,
"name": "PSF_NUM_R",
"pretty_name": null,
"description": "PSFEx number of stars used",
"documentation": "",
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.464569Z",
"updated": "2021-02-09T04:07:53.681755Z",
"contact": null,
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},
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"id": 1285,
"name": "PSF_NUM_U",
"pretty_name": null,
"description": "PSFEx number of stars used",
"documentation": "",
"file_path": null,
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"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:31.481874Z",
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]
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]
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"id": 12,
"name": "SpecCat",
"pretty_name": "SpecCat",
"description": "This DMU provides the final spectra and redshift catalogues, including GAMA AAT and external data.",
"documentation": "SpecCat<br>2011-07-21<br>Joe Liske <jliske@eso.org><br><br>This DMU produces the final spectra and redshift catalogues.<br><br>The 2dF/AAOmega multi-fibre instrument on the 3.9m Anglo-Australian<br>Telescope (AAT) is the main source of spectroscopic data for the GAMA<br>survey. Observations for GAMA I, part of which are released in DR2,<br>extended over three years (2008 - 2010, referred to below as Y1, Y2,<br>Y3). <br><br>The table AATFields provided by this DMU lists all 392 AAT 2dF/AAOmega<br>observations (fields) observed for GAMA I. Each of these observations<br>delivered on average 345 spectra of galaxy targets (for details of the<br>data, the observing and data reduction procedures, please see Hopkins<br>et al. 2013). AATFields provides some basic information on each<br>observation, including some rudimentary redshift success statistics.<br><br>All spectra collected for GAMA at the AAT were redshifted at the<br>telescope using the code runz (see below for a brief description of<br>this process). In addition, a fair fraction of the spectra were<br>redshifted again subsequently, some multiple times. The table<br>AATRunzResults contains the complete redshifting results<br>(i.e. essentially the runz output) for all GAMA AAT spectra that are<br>part of DR2.<br><br>The table AATSpecAllzAll contains one line for each GAMA AAT spectrum<br>in this release, summarising all of the redshifting results for this<br>spectrum, as well as listing the results of the analysis to determine<br>the best redshift based on the reliabilities of the redshifters. (The<br>reliabilities of the redshifters were determined in an analysis of the<br>re-redshifting results.)<br><br>The table AATSpecAll contains one line for each GAMA AAT spectrum<br>included in DR2, giving its best redshift as well as listing a number<br>of other properties of the spectrum, including its location on the<br>file server. Note that duplicate observations of the same objects are<br>retained in this table.<br><br>The table LTSpecAll lists a small number of spectra of fibre-bright<br>targets collected by the GAMA team at the Liverpool Telescope (LT).<br><br>The table SpecAll combines the tables AATSpecAll and LTSpecAll above<br>with the tables ExternalSpecAll and ExternalzAll from the <a href=\"/dr2/schema/dmu.php?name=ExternalSpec\">ExternalSpec<br>DMU</a>, thus providing a complete list of all spectra and redshifts that<br>are available for the objects included in DR2, including GAMA spectra<br>and those from previous spectroscopic surveys (such as the SDSS). Note<br>that duplicate observations of the same object are still retained in<br>this table. Note further that for those entries originating from<br>ExternalzAll table some parameters are not defined (such as e.g. the<br>minimum and maximum wavelengths of the spectrum).<br><br>Finally, the table SpecObj contains one line for each object in<br>SpecAll, giving details of the spectrum that provides the best<br>redshift (GAMA or otherwise), including the redshift. This is the<br>table we expect most users will be most interested in. Note that this<br>table contains 72,213 objects, which is 12 fewer than the number of<br>objects nominally included in DR2. For these 12 objects GAMA I simply<br>contains no spectroscopic or redshift data.<br><br>More information on particular aspects of these tables is given below.<br><br><br>----------------------------------------------------------------------<br><br><br>DMU dependencies<br>----------------<br>This version of the SpecCat DMU made use of the outputs of the<br>following DMUs:<br><br>Data/redshifting reduced_08 (comprising Y1-Y3 data)<br> See the GAMA file server and Hopkins et al. (2013) <br> for details on the data and data reduction procedures.<br>Re-redshifting v02 (covering Y1-Y3 data)<br>InputCat v16<br>ExternalSpec v01<br><br>Note that re-redshifting v02 did not fully complete the re-redshifting<br>of the Y3 data, leaving about 10% of the data that were not<br>re-redshifted.<br><br><br>Redshifting<br>-----------<br>All spectra observed for GAMA with the AAT are 'redshifted' by the<br>observing team at the telescope. The process of redshifting an<br>observation involves running the program 'runz' on a reduced data file<br>(typically containing ~345 spectra). For each spectrum, runz<br>automatically estimates a redshift, and then displays the spectrum<br>along with the positions of a number of common emission and absorption<br>lines at the estimated redshift. The job of the redshifter is now to<br>check whether the automatically determined redshift is correct. If<br>not, the user tries to find the correct redshift him/herself using a<br>number of methods provided by runz. The user then explicitly assigns a<br>quality, QOP (sometimes referred to as just Q), to the redshift before<br>moving on to the next spectrum. QOP can take values 0-4 with the<br>following meanings:<br><br>QOP = 4: The redshift is certainly correct.<br>QOP = 3: The redshift is probably correct.<br>QOP = 2: The redshift may be correct. Must be checked before being <br> included in a scientific analysis.<br>QOP = 1: No redshift could be found.<br>QOP = 0: Complete data reduction failure.<br><br>The output of the runz code is stored in table AATRunzResults.<br><br><br>The meaning of QOP=1 and 2 in early data<br>----------------------------------------<br>Note that there was a change in the meaning of the user-assigned<br>redshift quality values QOP=1 and 2 between year 2 and year 3 of the<br>GAMA I observing campaign. In Y1 and Y2 data QOP=1 was not used and<br>the meaning of QOP=2 is different from its meaning in later data. This<br>affects only table AATRunzResults. In table AATSpecAllzAll all the old<br>Y1+2 QOP=2 values were translated to the new QOP=1 and 2 values.<br><br><br>Re-redshifting<br>--------------<br>All QOP=1,2,3 and some QOP=4 data from Y1, Y2 and Y3 have been<br>independently re-redshifted by other GAMA team members (where the Y3<br>re-redshifting is not entirely complete). This provided additional<br>independent opinion(s) for each re-redshifted spectrum, as well as<br>estimates of how reliably each redshifter performed. This information<br>was used to produce a new, normalised redshift quality scale (called<br>nQ). This has been applied to all available redshift information (see<br>table AATSpecAllzAll). The quality of the redshift data is hence<br>largely homogeneous (except for the small incompleteness of the Y3<br>re-redshifting).<br><br><br>SPECID<br>------<br>All tables in this DMU make use of this parameter to identify a given<br>spectrum. For GAMA AAT spectra this is simply given by FIELDID_nnn<br>where nnn is the fibre number. See the notes of the ExternalSpec DMU<br>on how SPECID is defined for spectra from previous surveys.<br><br><br>Matching spectra to objects<br>---------------------------<br>Spectra are associated with GAMA objects by positionally matching them<br>to objects in the input catalogues, i.e. we do not simply use the IDs<br>of objects as provided in the 2dF/AAOmega configuration files. This is<br>done (i) because for a small sub-set of targets the ID changed<br>subsequent to the observations, and (ii) to match the procedure<br>employed by the ExternalSpec DMU.<br><br>For a given spectrum a matching GAMA object was identified by finding<br>the spectrum's closest GAMA object (within 1 arcsec) in the catalogue<br>resulting from the union of TilingCat and SpStandards. For those<br>spectra left without a match we then identified the closest GAMA<br>object (within 2 arcsec) in InputCatA.<br><br>Matched objects are identified by their CATAID and GAMA_NAME. The<br>parameter IC_FLAG is a bitwise flag identifying the catalogue(s) in<br>which the matched GAMA object was found:<br><br> Bit n 2^(n-1) Catalogue<br> -------------------------------<br> 1 1 InputCatA\t<br> 2 2 TilingCat<br> 3 4 SpStandards<br><br>The distance between a spectrum and its matched object in arcsec is<br>given by the parameter DIST.<br><br>In cases where multiple GAMA spectra were matched to the same GAMA<br>object (duplicate observations) the flag IS_SBEST in table AATSpecAll<br>identifies the spectrum providing the best redshift for that<br>object. This spectrum was identified first by nQ, and then (in cases<br>of multiple spectra with the same nQ) by the parameter PROB-DIST.<br><br>In cases where multiple GAMA and non-GAMA spectra were matched to the<br>same GAMA object the flag IS_BEST in table SpecAll identifies the<br>spectrum providing the best redshift for that object. This spectrum<br>was identified by considering only spectra with IS_SBEST=T and then<br>selecting first by nQ, and then (in cases of multiple spectra with the<br>same nQ) by the parameter PROB-DIST.<br><br>",
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"type": "CatalogueGroup",
"created": "2021-01-28T00:39:53.152982Z",
"updated": "2021-02-09T04:07:34.516979Z",
"contact": {
"email": "jliske@eso.org",
"name": "Joe Liske "
},
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"id": 35,
"name": "LTSpecAll",
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"description": "This table lists a small number of spectra of fibre-bright targets collected by the GAMA team at the Liverpool Telescope (LT).",
"documentation": "",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/LTSpecAll.fits",
"file_name": "LTSpecAll.fits",
"file_extension": "fits",
"version": "v01",
"type": "CatalogueTable",
"created": "2021-01-28T00:39:54.200671Z",
"updated": "2021-02-09T04:07:35.107572Z",
"contact": {
"email": "jliske@eso.org",
"name": "Joe Liske "
},
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"id": 1632,
"name": "CATAID",
"pretty_name": null,
"description": "ID of matched GAMA object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.581159Z",
"updated": "2021-02-09T04:07:58.613725Z",
"contact": null,
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},
{
"id": 1633,
"name": "DEC",
"pretty_name": null,
"description": "DEC of spectrum (J2000)",
"documentation": "",
"file_path": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.616939Z",
"updated": "2021-02-09T04:07:58.625916Z",
"contact": null,
"ucd": "pos.eq.dec",
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},
{
"id": 1635,
"name": "FILENAME",
"pretty_name": null,
"description": "Full path and filename of the spectrum",
"documentation": "",
"file_path": null,
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"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.671631Z",
"updated": "2021-02-09T04:07:58.652305Z",
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"id": 1636,
"name": "GAMA_NAME",
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"description": "Name of matched GAMA object",
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"created": "2021-01-28T00:40:40.692510Z",
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"id": 1637,
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"description": "Catalogue source(s) of matched GAMA object",
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"created": "2021-01-28T00:40:40.785003Z",
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"id": 1638,
"name": "IS_SBEST",
"pretty_name": null,
"description": "Is this the best GAMA LT spectrum of this object?",
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"created": "2021-01-28T00:40:40.812290Z",
"updated": "2021-02-09T04:07:58.691144Z",
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},
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"id": 1639,
"name": "NQ",
"pretty_name": null,
"description": "Normalised redshift quality (use nQ > 2 for science)",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.836001Z",
"updated": "2021-02-09T04:07:58.703491Z",
"contact": null,
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},
{
"id": 1640,
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"pretty_name": null,
"description": "Probability that redshift is correct",
"documentation": "",
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.863222Z",
"updated": "2021-02-09T04:07:58.717112Z",
"contact": null,
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},
{
"id": 1641,
"name": "RA",
"pretty_name": null,
"description": "RA of spectrum (J2000)",
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"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.898959Z",
"updated": "2021-02-09T04:07:58.730289Z",
"contact": null,
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},
{
"id": 1642,
"name": "SPECID",
"pretty_name": null,
"description": "ID of GAMA LT spectrum",
"documentation": "",
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.919484Z",
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},
{
"id": 1643,
"name": "URL",
"pretty_name": null,
"description": "URL of the spectrum",
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"version": null,
"type": "CatalogueColumn",
"created": "2021-01-28T00:40:40.953832Z",
"updated": "2021-02-09T04:07:58.756271Z",
"contact": null,
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},
{
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{
"id": 14,
"name": "StellarMasses",
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"description": "This DMU provides stellar masses, restframe photometry, and other ancillary stellar population parameters for all z < 0.65 galaxies in the GAMA DR2 sample.",
"documentation": "StellarMasses<br>StellarMasses<br>v08<br>2012-12-07<br>Edward Taylor <ent@physics.usyd.edu.au><br><br>This table provides stellar masses, restframe photometry, and other<br>ancillary stellar population parameters from stellar population fits<br>to ugriz SEDs for all galaxies with 0 < z < 0.65 and nQ > 1 from the<br>GAMA DR2 sample. Maximum redshifts for target selection are also<br>given, for use in 1/Vmax-style incompleteness corrections.<br><br>VERY IMPORTANT NOTE:<br>The values in this table are based on aperture (AUTO) photometry,<br>which may miss a significant fraction of a galaxy's light. Make sure<br>you understand the need for and meaning of the quantity <fluxscale>,<br>which is described under 'based on matched aperture photometry' below.<br><br>When using this table, please refer to:<br><a href=\"http://adsabs.harvard.edu/abs/2011MNRAS.418.1587T\">E.N. Taylor et al., 2011, MNRAS, 418, 1587</a><br>______________________________________________________________________________<br><br>DMU dependencies:<br>\tTilingCat\t\t- heliocentric redshifts, quality flags, etc.<br>\tApMatchedCat\t\t- matched aperture SED photometry<br>\tSersicCatAll\t\t- total r-band Sersic magnitudes<br>\tGalacticExtinction\t- foreground dust values<br>\tDistancesFrames\t\t- flow corrected redshifts for distances<br>______________________________________________________________________________<br><br><br><br>STELLAR POPULATION SYNTHESIS MODELLING: ______________________________________<br><br>The data provided by this table have been derived through stellar<br>population synthesis modelling of broadband optical (ugriz)<br>photometry. The modelling is done using the Bruzual & Charlot (2003)<br>stellar evolution models, assuming a Chabrier (2003) stellar initial<br>mass function (IMF) and the Calzetti et al. (2000) dust curve. The SPS<br>models used in the fitting are defined via four parameters: e-folding<br>time for the (exponentially declining) star formation history, time<br>since formation (ie. age), stellar metallicity, and dust attenuation<br>(Section 3.1 of Taylor et al. 2011). Note that the NIR photometry<br>available for GAMA galaxies have not been used at this stage, for the<br>simple reason that the models do not provide a good description of the<br>full optical-to-NIR SED shapes (Section 4 of Taylor et al. 2011). The<br>SPS grid spans the range 0 < z < 0.65; objects with z > 0.65 have not<br>been fit. (Talk to Edward Taylor if you need/would like mass estimates<br>for these galaxies.) The values of all derived parameters given in<br>the table, including the formal uncertainties, have been derived in a<br>Bayesian way (Sections 3.2-3.4 of Taylor et al. 2011).<br><br>DISTANCES AND COSMOLOGY: _____________________________________________________<br><br>All values are derived for the concordance (Omega_m, Omega_L, h) =<br>(0.3, 0.7, 0.7) cosmology. Stellar population parameters including<br>ages, dust extinctions, and mass-to-light ratios are cosmology<br>independent, inasmuch as they pertain to the stellar populations at<br>the time of observation. Restframe luminosities and thus the total<br>stellar mass do depend on distance, and so on h^-2. These can be<br>scaled in the usual way, such that a higher value of h implies a lower<br>distance, and thus a lower luminosity/mass (see below). Note that<br>distances have been computed using the flow-corrected redshifts<br><Z_TONRY> given in DistancesFrames. These values have been derived<br>using the Tonry et al. (2000) flow model for very low redshifts, and<br>then tapering to a CMB-centric frame for z > 0.03, as described by<br>Baldry et al. (2012), and are reproduced in this catalogue.<br><br>BASED ON MATCHED APERTURE PHOTOMETRY: ________________________________________<br><br>The results given have been derived from ugriz SEDs constructed from<br>matched aperture photometry. The photometry is the r-defined AUTO<br>photometry from ApMatchedCat (see Hill et al. 2011; Liske et al. in<br>prep.)<br><br>AN APERTURE CORRECTION IS THEREFORE REQUIRED for integrated quantities<br>(i.e. stellar mass or luminosity), in order to account for mass/flux<br>that falls beyond the finite AUTO aperture used for the SEDs. The<br>column <fluxscale> is provided for this purpose. The quantity<br><fluxscale> is the (linear) ratio between the r-band (AUTO) aperture<br>flux and the total r-band flux inferred from fitting a Sersic profile<br>(truncated at 10 Re, i.e. <GAL_MAG_10RE_R> from SersicCatAll).<br><br>THIS CORRECTION IS NOT APPLIED BY DEFAULT for two reasons. First, not<br>all objects have a Sersic-fit magnitude owing to failures in either<br>the SExtractor detection/segmentation or the GALFIT Sersic fitting<br>procedures (see Kelvin et al. 2012). These objects can be identified<br>as those with <fluxscale> = -9999. (Note that there is also 1 object<br>that Source Extractor has failed to produce r-band AUTO photometry<br>for, which is given <fluxscale> = 9999.) Second, particularly for the<br>fainter galaxies with higher (but unquantified) uncertainties in the<br>Sersic-fit magnitudes, the flux scaling implied by the Sersic<br>magnitudes is not necessarily physically sensible. For many galaxies,<br>the Sersic magnitude is less than the aperture magnitude, which is<br>logically inconsistent. Further, for some galaxies, the implied flux<br>scaling leads to masses that are unrealistically high (log M* >> 13).<br><br>THE USER IS THEREFORE TRUSTED TO APPLY THESE CORRECTIONS, but with the<br>understanding that some care is required. The recommended mass to use<br>is thus:<br> log10 M*,total = <logmstar> + log10(<fluxscale>) - 2 log10(h/0.7), <br>and the recommended absolute magnitudes in the X-band are:<br> M_X,total = <absmag_X> - 2.5 log10(<fluxscale>) + 5 log10(h/0.7).<br><br>Users should check to ensure that this makes sense (e.g. check that<br><fluxscale> is greater than or equal to unity, and that the magnitude<br>of the correction is not a factor of many) for their specific<br>object(s) of interest. Note, too, that this correction introduces an<br>additional source of uncertainty in the total luminosities and masses<br>that is not quantified in these tables.<br><br>RESTFRAME PHOTOMETRY AND COLOURS: ____________________________________________<br><br>All of the photometry provided by this table has been inferred from<br>the SPS fits as an attribute of the SP models. All restframe<br>photometry uses AB zeropoints and is k-corrected to redshift 0, with<br>no evolution corrections. The table contains restframe (g - i) and (u<br>- r) colours (in the columns <gminusi> and <uminusi>, respectively) as<br>well as restframe photometry in individual bands (e.g. <absmag_g> and<br><absmag_i>). Because in the fitting process, ugriz fluxes are highly<br>correlated with one another, the formal uncertainties on <gminusi> or<br><uminusr> cannot in general be derived from the <delrfphot>s. It is<br>thus preferable to use, e.g., <gminusi> and the associated uncertainty<br><delgminusi> rather than <absmag_g> - <absmag_i>.<br><br>INTRINSIC VERSUS EFFECTIVE RESTFRAME PHOTOMETRY: _____________________________<br><br>The quantities <absmag_X> should be understood as *effective*<br>restframe absolute magnitudes in the X-band; that is, the absolute<br>magnitudes corresponding to the light the observer actually sees from<br>the galaxy, without correction for extinction within the galaxy<br>itself. In contrast, the quantites <absmag_X_stars> give *intrinsic*<br>absolute magnitudes in the X-band, which should be understood to be<br>the total light emitted by stars; that is, corrected for internal dust<br>extinction according to <extBV>. In both cases, these values are<br>derived from the SPS fits as properties of the stellar populations in<br>a similar way to ages, metallicities, mass-to-light ratios,<br>etc. (i.e. a la Equation 5 of Taylor et al. 2011).<br><br>MAXIMAL DETECTION/SELECTION REDSHIFTS FOR INCOMPLETENESS CORRECTIONS: ________<br><br>In order to facilitate the derivation of completeness-corrected number<br>densities, limiting redshifts have been derived for three r-band<br>selection limits: r < 17.88 (i.e. SDSS main sample target selection);<br>r < 19.4 (G09 and G15 SURVEY_CLASS >= 6 target selection); and r <<br>19.8 (G12 SURVEY_CLASS >= 6 target selection). All three of these<br>selections are phrased in terms of r-band Petrosian magnitudes, as<br>given in the SDSS DR6 catalogues, AFTER correction for foreground<br>(Galactic) extinction, and quoted as <R_PETRO> in TilingCatv16. The<br>limiting redshifts are the maximum redshift at which any given galaxy<br>would satisfy the r-band selection in question. These values have been<br>derived in the course of the SPS fits, using the single best fitting<br>template to estimate how the r-band magnitude varies with<br>redshift/distance. Note that these limiting redshifts should be<br>understood as being flow-corrected, not heliocentric (see Section 3.5<br>of Taylor et al. 2011). Users should bear this in mind when selecting<br>or binning galaxies by redshift. As an example for how to use these<br>values, imagining that the user is considering galaxies with z <<br>z_limit, the effective survey volume for each individual object can be<br>calculated as:<br><br> V_max ~ 96 * comovingVolume(min(zmax_19p4, zlimit)) <br>\t+ 48 * comovingVolume(min(zmax_19p8, zlimit)).<br><br>Talk to, for example, Edward Taylor, Ivan Baldry, or Peder Norberg if<br>you are worried about how to do this.<br><br>KNOWN ISSUES: ________________________________________________________________<br><br>* There are a number of very low redshift objects that are given<br> unphysically low values for <logmstar>; e.g. <logmstar> << 6. These<br> are almost all stars, and can largely be excluded by considering z ><br> 0.003.<br><br>* There are a very few objects for which the fitting procedure has<br> failed. For these objects, all SP parameters are given as -99;<br> i.e. as missing data.<br><br>* There are a number of objects that are given one or more of the<br> <zmax>s >= 0.65. This corresponds to the maximum redshift covered by<br> the SPL grid. This is true for many of the galaxies where the fits<br> have failed (see above), but also for galaxies with reasonable SP<br> parameters. For these \"okay\" galaxies, this should be interpreted as<br> a lower limit to the values of the <zmax>s. (Or, in other words, the<br> implication is that GAMA is volume limited for such objects for z <=<br> 0.65.)<br><br>* There are a number of objects with Z ~ 0.05, which corresponds to<br> the maximum metallicity contained in the SPS grids. The mass<br> estimates for these objects are unlikely to be significantly<br> compromised, but the age and dust extinction values may be biased.<br><br>",
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{
"id": 42,
"name": "StellarMasses",
"pretty_name": null,
"description": "This table provides stellar masses, restframe photometry, and other ancillary stellar population parameters from stellar population fits to ugriz SEDs for all z < 0.65 galaxies in the GAMA DR2 sample.",
"documentation": "StellarMasses<br>StellarMasses<br>v08<br>2012-12-07<br>Edward Taylor <ent@physics.usyd.edu.au><br><br>This table provides stellar masses, restframe photometry, and other<br>ancillary stellar population parameters from stellar population fits<br>to ugriz SEDs for all galaxies with 0 < z < 0.65 and nQ > 1 from the<br>GAMA DR2 sample. Maximum redshifts for target selection are also<br>given, for use in 1/Vmax-style incompleteness corrections.<br><br>VERY IMPORTANT NOTE:<br>The values in this table are based on aperture (AUTO) photometry,<br>which may miss a significant fraction of a galaxy's light. Make sure<br>you understand the need for and meaning of the quantity <fluxscale>,<br>which is described under 'based on matched aperture photometry' below.<br><br>When using this table, please refer to:<br><a href=\"http://adsabs.harvard.edu/abs/2011MNRAS.418.1587T\">E.N. Taylor et al., 2011, MNRAS, 418, 1587</a><br>______________________________________________________________________________<br><br>DMU dependencies:<br>\tTilingCat\t\t- heliocentric redshifts, quality flags, etc.<br>\tApMatchedCat\t\t- matched aperture SED photometry<br>\tSersicCatAll\t\t- total r-band Sersic magnitudes<br>\tGalacticExtinction\t- foreground dust values<br>\tDistancesFrames\t\t- flow corrected redshifts for distances<br>______________________________________________________________________________<br><br><br><br>STELLAR POPULATION SYNTHESIS MODELLING: ______________________________________<br><br>The data provided by this table have been derived through stellar<br>population synthesis modelling of broadband optical (ugriz)<br>photometry. The modelling is done using the Bruzual & Charlot (2003)<br>stellar evolution models, assuming a Chabrier (2003) stellar initial<br>mass function (IMF) and the Calzetti et al. (2000) dust curve. The SPS<br>models used in the fitting are defined via four parameters: e-folding<br>time for the (exponentially declining) star formation history, time<br>since formation (ie. age), stellar metallicity, and dust attenuation<br>(Section 3.1 of Taylor et al. 2011). Note that the NIR photometry<br>available for GAMA galaxies have not been used at this stage, for the<br>simple reason that the models do not provide a good description of the<br>full optical-to-NIR SED shapes (Section 4 of Taylor et al. 2011). The<br>SPS grid spans the range 0 < z < 0.65; objects with z > 0.65 have not<br>been fit. (Talk to Edward Taylor if you need/would like mass estimates<br>for these galaxies.) The values of all derived parameters given in<br>the table, including the formal uncertainties, have been derived in a<br>Bayesian way (Sections 3.2-3.4 of Taylor et al. 2011).<br><br>DISTANCES AND COSMOLOGY: _____________________________________________________<br><br>All values are derived for the concordance (Omega_m, Omega_L, h) =<br>(0.3, 0.7, 0.7) cosmology. Stellar population parameters including<br>ages, dust extinctions, and mass-to-light ratios are cosmology<br>independent, inasmuch as they pertain to the stellar populations at<br>the time of observation. Restframe luminosities and thus the total<br>stellar mass do depend on distance, and so on h^-2. These can be<br>scaled in the usual way, such that a higher value of h implies a lower<br>distance, and thus a lower luminosity/mass (see below). Note that<br>distances have been computed using the flow-corrected redshifts<br><Z_TONRY> given in DistancesFrames. These values have been derived<br>using the Tonry et al. (2000) flow model for very low redshifts, and<br>then tapering to a CMB-centric frame for z > 0.03, as described by<br>Baldry et al. (2012), and are reproduced in this catalogue.<br><br>BASED ON MATCHED APERTURE PHOTOMETRY: ________________________________________<br><br>The results given have been derived from ugriz SEDs constructed from<br>matched aperture photometry. The photometry is the r-defined AUTO<br>photometry from ApMatchedCat (see Hill et al. 2011; Liske et al. in<br>prep.)<br><br>AN APERTURE CORRECTION IS THEREFORE REQUIRED for integrated quantities<br>(i.e. stellar mass or luminosity), in order to account for mass/flux<br>that falls beyond the finite AUTO aperture used for the SEDs. The<br>column <fluxscale> is provided for this purpose. The quantity<br><fluxscale> is the (linear) ratio between the r-band (AUTO) aperture<br>flux and the total r-band flux inferred from fitting a Sersic profile<br>(truncated at 10 Re, i.e. <GAL_MAG_10RE_R> from SersicCatAll).<br><br>THIS CORRECTION IS NOT APPLIED BY DEFAULT for two reasons. First, not<br>all objects have a Sersic-fit magnitude owing to failures in either<br>the SExtractor detection/segmentation or the GALFIT Sersic fitting<br>procedures (see Kelvin et al. 2012). These objects can be identified<br>as those with <fluxscale> = -9999. (Note that there is also 1 object<br>that Source Extractor has failed to produce r-band AUTO photometry<br>for, which is given <fluxscale> = 9999.) Second, particularly for the<br>fainter galaxies with higher (but unquantified) uncertainties in the<br>Sersic-fit magnitudes, the flux scaling implied by the Sersic<br>magnitudes is not necessarily physically sensible. For many galaxies,<br>the Sersic magnitude is less than the aperture magnitude, which is<br>logically inconsistent. Further, for some galaxies, the implied flux<br>scaling leads to masses that are unrealistically high (log M* >> 13).<br><br>THE USER IS THEREFORE TRUSTED TO APPLY THESE CORRECTIONS, but with the<br>understanding that some care is required. The recommended mass to use<br>is thus:<br> log10 M*,total = <logmstar> + log10(<fluxscale>) - 2 log10(h/0.7), <br>and the recommended absolute magnitudes in the X-band are:<br> M_X,total = <absmag_X> - 2.5 log10(<fluxscale>) + 5 log10(h/0.7).<br><br>Users should check to ensure that this makes sense (e.g. check that<br><fluxscale> is greater than or equal to unity, and that the magnitude<br>of the correction is not a factor of many) for their specific<br>object(s) of interest. Note, too, that this correction introduces an<br>additional source of uncertainty in the total luminosities and masses<br>that is not quantified in these tables.<br><br>RESTFRAME PHOTOMETRY AND COLOURS: ____________________________________________<br><br>All of the photometry provided by this table has been inferred from<br>the SPS fits as an attribute of the SP models. All restframe<br>photometry uses AB zeropoints and is k-corrected to redshift 0, with<br>no evolution corrections. The table contains restframe (g - i) and (u<br>- r) colours (in the columns <gminusi> and <uminusi>, respectively) as<br>well as restframe photometry in individual bands (e.g. <absmag_g> and<br><absmag_i>). Because in the fitting process, ugriz fluxes are highly<br>correlated with one another, the formal uncertainties on <gminusi> or<br><uminusr> cannot in general be derived from the <delrfphot>s. It is<br>thus preferable to use, e.g., <gminusi> and the associated uncertainty<br><delgminusi> rather than <absmag_g> - <absmag_i>.<br><br>INTRINSIC VERSUS EFFECTIVE RESTFRAME PHOTOMETRY: _____________________________<br><br>The quantities <absmag_X> should be understood as *effective*<br>restframe absolute magnitudes in the X-band; that is, the absolute<br>magnitudes corresponding to the light the observer actually sees from<br>the galaxy, without correction for extinction within the galaxy<br>itself. In contrast, the quantites <absmag_X_stars> give *intrinsic*<br>absolute magnitudes in the X-band, which should be understood to be<br>the total light emitted by stars; that is, corrected for internal dust<br>extinction according to <extBV>. In both cases, these values are<br>derived from the SPS fits as properties of the stellar populations in<br>a similar way to ages, metallicities, mass-to-light ratios,<br>etc. (i.e. a la Equation 5 of Taylor et al. 2011).<br><br>MAXIMAL DETECTION/SELECTION REDSHIFTS FOR INCOMPLETENESS CORRECTIONS: ________<br><br>In order to facilitate the derivation of completeness-corrected number<br>densities, limiting redshifts have been derived for three r-band<br>selection limits: r < 17.88 (i.e. SDSS main sample target selection);<br>r < 19.4 (G09 and G15 SURVEY_CLASS >= 6 target selection); and r <<br>19.8 (G12 SURVEY_CLASS >= 6 target selection). All three of these<br>selections are phrased in terms of r-band Petrosian magnitudes, as<br>given in the SDSS DR6 catalogues, AFTER correction for foreground<br>(Galactic) extinction, and quoted as <R_PETRO> in TilingCatv16. The<br>limiting redshifts are the maximum redshift at which any given galaxy<br>would satisfy the r-band selection in question. These values have been<br>derived in the course of the SPS fits, using the single best fitting<br>template to estimate how the r-band magnitude varies with<br>redshift/distance. Note that these limiting redshifts should be<br>understood as being flow-corrected, not heliocentric (see Section 3.5<br>of Taylor et al. 2011). Users should bear this in mind when selecting<br>or binning galaxies by redshift. As an example for how to use these<br>values, imagining that the user is considering galaxies with z <<br>z_limit, the effective survey volume for each individual object can be<br>calculated as:<br><br> V_max ~ 96 * comovingVolume(min(zmax_19p4, zlimit)) <br>\t+ 48 * comovingVolume(min(zmax_19p8, zlimit)).<br><br>Talk to, for example, Edward Taylor, Ivan Baldry, or Peder Norberg if<br>you are worried about how to do this.<br><br>KNOWN ISSUES: ________________________________________________________________<br><br>* There are a number of very low redshift objects that are given<br> unphysically low values for <logmstar>; e.g. <logmstar> << 6. These<br> are almost all stars, and can largely be excluded by considering z ><br> 0.003.<br><br>* There are a very few objects for which the fitting procedure has<br> failed. For these objects, all SP parameters are given as -99;<br> i.e. as missing data.<br><br>* There are a number of objects that are given one or more of the<br> <zmax>s >= 0.65. This corresponds to the maximum redshift covered by<br> the SPL grid. This is true for many of the galaxies where the fits<br> have failed (see above), but also for galaxies with reasonable SP<br> parameters. For these \"okay\" galaxies, this should be interpreted as<br> a lower limit to the values of the <zmax>s. (Or, in other words, the<br> implication is that GAMA is volume limited for such objects for z <=<br> 0.65.)<br><br>* There are a number of objects with Z ~ 0.05, which corresponds to<br> the maximum metallicity contained in the SPS grids. The mass<br> estimates for these objects are unlikely to be significantly<br> compromised, but the age and dust extinction values may be biased.<br><br>",
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"documentation": "kCorrections<br>2012-09-24<br>Jon Loveday <j.loveday@sussex.ac.uk><br><br>This DMU provides k-corrections in the GALEX FUV and NUV bands, the<br>SDSS ugriz bands and the UKIDSS YJHK bands for all GAMA DR2 galaxies.<br>The k-corrections were calculated with <a href=\"http://howdy.physics.nyu.edu/index.php/Kcorrect\">kcorrect v4_2</a> using SDSS<br>DR6 model magnitudes. Please see <a href=\"http://adsabs.harvard.edu/abs/2007AJ....133..734B\">Blanton & Roweis (2007)</a> for further<br>information on kcorrect, its output and its performance. In<br>particular, see Section 3.4 of that paper if you plan to use the UV or<br>NIR k-corrections.<br><br>K-corrections are provided for both redshift 0.0 (table kcorr_z00)<br>and for redshift 0.1 (table kcorr_z01).<br><br>The corrections were calculated for all GAMA DR2 galaxies with<br>nQ >= 2 using Z_TONRY from DistancesFrames. However, they will be<br>meaningless for negative redshifts. Note that, strictly speaking,<br>geocentric redshifts should be used to calculate k-corrections, but<br>here we have used Tonry flow-corrected redshifts for consistency with<br>Vmax calculations.<br><br>The tables in this DMU also provide the coefficients of a polynomial<br>fit to the k-corrections in the columns PCOEFF_X_* (see <a href=\"http://adsabs.harvard.edu/abs/2012MNRAS.420.1239L\">Loveday et<br>al. (2012)</a> for details). These coefficients are ordered high to low<br>order, such that<br>KCORR_X(z) = sum_{i=1}^5 PCOEFF_*_i * (z - zRef)^(5-i)<br>or for python users<br>KCORR_X(z) = numpy.polyval(PCOEFF_X_*, z - zRef)<br>where zRef = 0.0 for kcorr_z00 and zRef = 0.1 for kcorr_z01.<br><br>Note that the parameter PCOEFF_X_5 is fit for and is not kept<br>constant. Thus, the value of KCORR_X(zRef) provided by the polynomial<br>fits will in general not be equal to -2.5 log10(1+zRef), the value it<br>should have in principle.<br><br>In the <a href=\"/dr2/data/cat/kCorrections/v02/\">download directory</a> for this DMU we also provide fits binary<br>versions of the two tables of this DMU with columns PCOEFF_X_* and<br>COEFFS_* as vector columns rather than split into separate columns.<br><br>Note that columns CHI2, MASS, INTSFH, METS, B300 and B1000 are outputs<br>of kcorrect. These represent the physical interpretation of kcorrect's<br>SED fits to the photometry. However, these parameters have not been<br>tested at all, and this DMU does not vouch for their reliability or<br>meaningfulness. Hence, their scientific use is discouraged (especially<br>in cases where more careful measurements are provided by other<br>DMUs). These parameters were included here only for completeness and<br>because they may prove to be useful in identifying objects for which<br>kcorrect's SED fits are implausible.<br><br>",
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"email": "j.loveday@sussex.ac.uk",
"name": "Jon Loveday "
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"email": "j.loveday@sussex.ac.uk",
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},
{
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"documentation": "",
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},
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},
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"documentation": "",
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},
{
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"version": null,
"type": "CatalogueColumn",
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},
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"description": "SDSS DR6 z-band model magnitude error",
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"version": null,
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},
{
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"description": "Flow corrected redshift using Tonry et al. model",
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},
{
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"pretty_name": null,
"description": "Fraction of the total star formation that has occurred in the last 1 Gyr",
"documentation": "",
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},
{
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"name": "PCOEFF_J_4",
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"description": "Coefficient of polynomial fit to K(z) in UKIDSS J band",
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"file_path": null,
"file_name": null,
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"version": null,
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"contact": null,
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}
]
}
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}
]
},
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"ifs": null,
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{
"id": 4,
"name": "2dfgrs",
"pretty_name": "2dFGRS",
"description": "All 2dFGRS spectra of GAMA DR2 objects obtained through the 2dFGRS query page.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "SpectraFacility",
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"created": "2021-02-09T04:08:06.482105Z",
"updated": "2021-02-09T04:08:06.496490Z",
"contact": null,
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}
]
},
{
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"description": "All 2SLAQ QSO spectra of GAMA DR2 objects obtained through the 2SLAQ QSO query page.",
"documentation": "<div>\nThis directory contains all <a href=\"http://www.2slaq.info/\">2SLAQ</a> QSO\nspectra of GAMA DR2 objects obtained through the <a href=\"http://www.physics.usyd.edu.au/2slaq/spec_search/2slaq_search.html\">2SLAQ\nQSO query page</a> The primary extension contains the spectrum, while the next extension\ncontains the variance.\n<br>\nSee also the <a href=\"/dr2/schema/dmu.php?name=ExternalSpec\">ExternalSpec DMU</a>.<br>\nThe sub-directory png/ contains a png image of each spectrum (black =\nspectrum, green = 1 sigma error array), smoothed with a boxcar of width 3 pixel.\n\n</div>",
"file_path": null,
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"type": "SpectraFacility",
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"contact": null,
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"name": "spectrum_1d",
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"file_path": null,
"file_name": null,
"file_extension": null,
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"type": "SpectrumDataProduct",
"created": "2021-02-09T04:08:06.578925Z",
"updated": "2021-02-09T04:08:06.593491Z",
"contact": null,
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}
]
},
{
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"description": "All GAMA I spectra of GAMA DR2 objects.",
"documentation": "<div>\nThis directory contains all GAMA I spectra of GAMA DR2 objects (reduced_08).\nThese fits files\ncontain the fully reduced and flux-calibrated spectrum, the reduced \nspectrum without the flux calibration, the corresponding error arrays, \nand the mean sky spectrum of the field from which this spectrum was taken. The files are named %s_%03d.fits (GAMA field name, fibre number).\n<br>\nThe sub-directory png/ contains a png image of each spectrum observed (black =\nflux-calibrated spectrum, green = 1 sigma error array, blue = sky spectrum), \nsmoothed with a boxcar of width 5 pixel.</div>",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "SpectraFacility",
"created": "2021-01-28T00:40:56.526495Z",
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"contact": null,
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"id": 50,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
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"documentation": "",
"file_path": null,
"file_name": null,
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"version": "v1.0",
"type": "SpectrumDataProduct",
"created": "2021-02-09T04:08:06.677785Z",
"updated": "2021-02-09T04:08:06.701720Z",
"contact": null,
"schema_key": "gama.dr2.spectra.gama.spectrum_1d"
}
]
},
{
"id": 10,
"name": "gama_lt",
"pretty_name": "GAMA LT",
"description": "A small number of spectra of bright objects obtained by the GAMA team using the Liverpool Telescope.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "SpectraFacility",
"created": "2021-01-28T00:40:56.544094Z",
"updated": "2021-02-09T04:08:06.428638Z",
"contact": null,
"data_products": [
{
"id": 51,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
"description": "Reduced 1D spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
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"created": "2021-02-09T04:08:06.732830Z",
"updated": "2021-02-09T04:08:06.756516Z",
"contact": null,
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}
]
},
{
"id": 5,
"name": "2qz",
"pretty_name": "2QZ",
"description": "All 2QZ spectra of GAMA DR2 objects obtained through the 2QZ query page.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "SpectraFacility",
"created": "2021-01-28T00:40:56.464039Z",
"updated": "2021-02-09T04:08:06.383643Z",
"contact": null,
"data_products": [
{
"id": 46,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
"description": "Reduced 1D spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v1.0",
"type": "SpectrumDataProduct",
"created": "2021-02-09T04:08:06.519689Z",
"updated": "2021-02-09T04:08:06.526596Z",
"contact": null,
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}
]
},
{
"id": 6,
"name": "2slaq-lrg",
"pretty_name": "2SLAQ LRG",
"description": "All 2SLAQ LRG spectra of GAMA DR2 objects obtained through the 2SLAQ LRG query page.",
"documentation": "<div>\nThis directory contains all <a href=\"http://www.2slaq.info/\">2SLAQ</a>\nLRG spectra of GAMA DR2 objects obtained through the <a href=\"http://2slaq.info/query/spec_search/\">2SLAQ LRG query page</a>.\n<br>\nSee also the <a href=\"/dr2/schema/dmu.php?name=ExternalSpec\">ExternalSpec DMU</a>.<br>\nThe sub-directory png/ contains a png image of each spectrum (black =\nspectrum, blue = arbitrarily scaled sky spectrum), smoothed with a boxcar \nof width 3 pixel.\n</div>",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "SpectraFacility",
"created": "2021-01-28T00:40:56.479504Z",
"updated": "2021-02-09T04:08:06.391433Z",
"contact": null,
"data_products": [
{
"id": 47,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
"description": "Reduced 1D spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v1.0",
"type": "SpectrumDataProduct",
"created": "2021-02-09T04:08:06.550616Z",
"updated": "2021-02-09T04:08:06.556693Z",
"contact": null,
"schema_key": "gama.dr2.spectra.2slaq-lrg.spectrum_1d"
}
]
},
{
"id": 8,
"name": "6dfgs",
"pretty_name": "6DFGS",
"description": "All 6DFGS spectra of GAMA DR2 objects obtained through the 6DFGS query page.",
"documentation": "<div>\nThis directory contains all <a href=\"http://www.aao.gov.au/local/www/6df/\">6dFGS</a> spectra of GAMA DR2 objects obtained through the <a href=\"http://www-wfau.roe.ac.uk/6dFGS/SQL.html\">6dFGS query page</a>.\nFrom the original <a href=\"http://www-wfau.roe.ac.uk/6dFGS/fits.html\">object fits files</a>\nprovided by the 6dFGS we have extracted and store only the combined VR\nspectra.\n<br>\nSee also the <a href=\"/dr2/schema/dmu.php?name=ExternalSpec\">ExternalSpec DMU</a>.<br>\nThe sub-directory png/ contains a png image of each spectrum (black =\nspectrum, green = 1 sigma error array, blue = arbitrarily scaled sky\nspectrum), smoothed with a boxcar of width 3 pixel.\n</div>",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "SpectraFacility",
"created": "2021-01-28T00:40:56.510936Z",
"updated": "2021-02-09T04:08:06.409898Z",
"contact": null,
"data_products": [
{
"id": 49,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
"description": "Reduced 1D spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v1.0",
"type": "SpectrumDataProduct",
"created": "2021-02-09T04:08:06.630809Z",
"updated": "2021-02-09T04:08:06.646699Z",
"contact": null,
"schema_key": "gama.dr2.spectra.6dfgs.spectrum_1d"
}
]
},
{
"id": 11,
"name": "mgc",
"pretty_name": "MGC",
"description": "All MGC spectra of GAMA DR2 objects.",
"documentation": "<div>\nThis directory contains all <a href=\"http://www.eso.org/~jliske/mgc/\">MGC</a> spectra of GAMA DR2 objects. From the original <a href=\"http://www.eso.org/~jliske/mgc/database.html\">object fits\nfiles</a> provided by the MGC we have extracted and store only the MGC\nspectra, although we have copied the photometric information\nprovided in the header of the original primary HDU to each\nspectrum. Duplicate observations are stored in separate files named\nMGCddddd_n.fit (where ddddd is the serial number of the MGC object\nand n the duplication index).\n<br>\nSee also the <a href=\"/dr2/schema/dmu.php?name=ExternalSpec\">ExternalSpec DMU</a>.<br>\nThe sub-directory png/ contains a png image of each spectrum (black =\nspectrum, green = 1 sigma error array, blue = arbitrarily scaled sky\nspectrum).\n</div>",
"file_path": null,
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"version": null,
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"created": "2021-01-28T00:40:56.560614Z",
"updated": "2021-02-09T04:08:06.438084Z",
"contact": null,
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"id": 52,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
"description": "Reduced 1D spectrum",
"documentation": "",
"file_path": null,
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"version": "v1.0",
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"created": "2021-02-09T04:08:06.788410Z",
"updated": "2021-02-09T04:08:06.811439Z",
"contact": null,
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}
]
},
{
"id": 12,
"name": "sdss",
"pretty_name": "SDSS",
"description": "All SDSS spectra of GAMA DR2 objects obtained through the SDSS SQL query page.",
"documentation": "<div>\nThis directory contains all <a href=\"http://www.sdss.org/\">SDSS</a>\nDR7 spectra of GAMA DR2 objects obtained through an <a href=\"http://cas.sdss.org/astrodr7/en/tools/search/SQL.asp\">SDSS SQL\nquery</a> on SpecObjAll. The only spectra that were excluded were\nthose with objType=22 (=SKY). The format of the fits files is\nexplained <a href=\"http://das.sdss.org/www/html/dm/flatFiles/spSpec.html\">here</a>\n<br>\nSee also the <a href=\"/dr2/schema/dmu.php?name=ExternalSpec\">ExternalSpec DMU</a>.<br>\nThe sub-directory png/ contains a png image of each spectrum (black =\nspectrum, green = 1 sigma error array), smoothed with a boxcar of width 5 pixel.\n</div>",
"file_path": null,
"file_name": null,
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"type": "SpectraFacility",
"created": "2021-01-28T00:40:56.616446Z",
"updated": "2021-02-09T04:08:06.446874Z",
"contact": null,
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"id": 53,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
"description": "Reduced 1D spectrum",
"documentation": "",
"file_path": null,
"file_name": null,
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"type": "SpectrumDataProduct",
"created": "2021-02-09T04:08:06.833692Z",
"updated": "2021-02-09T04:08:06.847721Z",
"contact": null,
"schema_key": "gama.dr2.spectra.sdss.spectrum_1d"
}
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},
{
"id": 13,
"name": "wigglez",
"pretty_name": "WiggleZ",
"description": "All WiggleZ spectra of GAMA DR2 objects obtained through the WiggleZ query page.",
"documentation": "<div>\nThis directory contains all <a href=\"http://wigglez.swin.edu.au/\">WiggleZ</a> DR1 spectra of\nGAMA DR2 objects (excluding duplicates) obtained through the WiggleZ <a href=\"http://wigglez.swin.edu.au/dr1/#/2\">query page</a>. Files are\nnamed Spectrum-n.fit, where n is a multiple digit number (the meaning\nof which in unclear). The primary extension contains the spectrum, the\nnext contains the noise, and the last extension contains the WiggleZ\ncatalogue data.\n<br>\nSee also the <a href=\"/dr2/schema/dmu.php?name=ExternalSpec\">ExternalSpec DMU</a>.<br>\nThe sub-directory png/ contains a png image of each spectrum (black =\nspectrum, green = 1 sigma error array), smoothed with a boxcar of width 5 pixel.\n</div>",
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"version": null,
"type": "SpectraFacility",
"created": "2021-01-28T00:40:56.652519Z",
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"contact": null,
"data_products": [
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"id": 54,
"name": "spectrum_1d",
"pretty_name": "1D Spectrum",
"description": "Reduced 1D spectrum",
"documentation": "",
"file_path": null,
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"created": "2021-02-09T04:08:06.870466Z",
"updated": "2021-02-09T04:08:06.875853Z",
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