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"url": "https://datacentral.org.au/api/schema/2/",
"name": "devils",
"pretty_name": "DEVILS",
"title": "The Deep Extragalactic VIsible Legacy Survey",
"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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{
"url": "https://datacentral.org.au/api/schema/3/",
"name": "gama",
"pretty_name": "GAMA",
"title": "Galaxy And Mass Assembly Survey",
"description": "<p>GAMA is a project to exploit the latest generation of ground-based and space-borne survey facilities to study cosmology and galaxy formation and evolution. </p> <p>At the heart of this project lies the GAMA spectroscopic survey of ~300,000 galaxies down to r < 19.8 mag over ~286 deg<sup>2</sup>, carried out using the <a href=\"http://www.aao.gov.au/AAO/2df/aaomega/aaomega.html\">AAOmega</a> multi-object spectrograph on the <a href=\"http://www.aao.gov.au/\">Anglo-Australian Telescope (AAT)</a> by the GAMA team</a>. This project was awarded 210 nights over 7 years (2008–2014) and the observations are now completed. This survey builds on, and is augmented by, previous spectroscopic surveys such as the <a href=\"http://www.sdss.org/\">Sloan Digital Sky Survey (SDSS)</a>, the <a href=\"http://www.mso.anu.edu.au/2dFGRS/\">2dF Galaxy Redshift Survey(2dFGRS)</a> and the <a href=\"http://www.eso.org/~jliske/mgc/\">Millennium Galaxy Catalogue (MGC)</a>.</p>",
"pi": "Simon Driver",
"contact": {
"email": "simon.driver@uwa.edu.au",
"name": "Simon Driver"
},
"website": "http://www.gama-survey.org/",
"active": true,
"type": "Survey",
"data_releases": [
{
"name": "dr2",
"pretty_name": "Data Release 2",
"version": 2.0,
"data_release_number": 2,
"contact": {
"email": "simon.driver@uwa.edu.au",
"name": "Simon Driver"
},
"created": "2020-07-28T01:34:50.191619Z",
"updated": "2020-08-10T01:21:28.568249Z",
"type": "DataRelease",
"catalogues": {
"groups": [
{
"id": 4,
"name": "ApMatchedPhotom",
"pretty_name": "ApMatchedPhotom",
"description": "This DMU provides aperture matched ugrizYJHK photometry.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": "v02",
"type": "CatalogueGroup",
"created": "2020-07-28T01:35:13.919840Z",
"updated": "2020-07-28T01:35:13.932965Z",
"contact": {
"email": "mehmet.alpaslan@icrar.org",
"name": "Mehmet Alpaslan "
},
"tables": [
{
"id": 4,
"name": "ApMatchedCat",
"pretty_name": null,
"description": "This table contains r-band aperture matched photometry and other Source Extractor outputs for all GAMA DR2 objects.",
"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.). In the meantime, users may wish to consider applying<br>the following zero-point offsets to bring the YJHK magnitudes of this<br>catalogue into agreement with VIKING:<br><br> Y_corr = Y_DR2 - 0.13 mag<br> J_corr = J_DR2 - 0.12 mag<br> H_corr = H_DR2 - 0.07 mag<br> K_corr = K_DR2 - 0.11 mag<br><br>########################################################################<br><br>Dependencies: <br><br>\tInputCat\tTilingCatv16 <br>\tMosaicing\tv02<br><br>#######################################################################<br><br>The Source Extractor parameters used to generate this catalogue are as <br>follows:<br><br>DETECT_MINAREA\t\t16\t<br>Minimum number of pixels above threshold triggering detection.<br><br>DETECT_THRESH\t\t1.7\t<br>Detection threshold relative to background.<br><br>FILTER\t\t\tN\t<br>If true, filtering is applied to the data before extraction.<br><br>DEBLEND_NTHRESH\t\t32\t<br>Number of deblending sub-thresholds. <br><br>DEBLEND_MINCONT\t0.00005\t<br>Minimum contrast parameter for deblending.<br><br>CLEAN_PARAM\t\t0.1<br>Efficiency of cleaning.<br><br>WEIGHT_TYPE\t\tNONE\t<br>Weighting scheme used for weight maps. 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>",
"file_path": "/data/ingestion_1.9/gama/dr2/catalogues/ApMatchedCat.fits",
"file_name": "ApMatchedCat.fits",
"file_extension": "fits",
"version": "v02",
"type": "CatalogueTable",
"created": "2020-07-28T01:35:14.398158Z",
"updated": "2020-07-28T01:35:14.412358Z",
"contact": {
"email": "mehmet.alpaslan@icrar.org",
"name": "Mehmet Alpaslan "
},
"input_cat": false,
"columns": [
{
"id": 177,
"name": "Y",
"pretty_name": null,
"description": "y coordinate of aperture centre in r band cutout",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:35:20.899371Z",
"updated": "2020-07-28T01:35:20.912025Z",
"contact": null,
"ucd": "pos",
"unit": "pixel"
},
{
"id": 176,
"name": "X",
"pretty_name": null,
"description": "x coordinate of aperture centre in r band cutout",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:35:20.871716Z",
"updated": "2020-07-28T01:35:20.884837Z",
"contact": null,
"ucd": "pos",
"unit": "pixel"
},
{
"id": 175,
"name": "THRESHOLD",
"pretty_name": null,
"description": "Detection threshold above background (r band)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:35:20.846889Z",
"updated": "2020-07-28T01:35:20.851670Z",
"contact": null,
"ucd": "instr.sensitivity;phot.count;em.opt.R",
"unit": "counts"
},
{
"id": 174,
"name": "THETA_J2000",
"pretty_name": null,
"description": "Position angle (east of north)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:35:20.811821Z",
"updated": "2020-07-28T01:35:20.824822Z",
"contact": null,
"ucd": "pos.posAng;em.opt.R",
"unit": "deg"
},
{
"id": 173,
"name": "THETA_IMAGE",
"pretty_name": null,
"description": "Position angle (counterclockwise)",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:35:20.778282Z",
"updated": "2020-07-28T01:35:20.791334Z",
"contact": null,
"ucd": "pos.posAng;em.opt.R",
"unit": "deg"
},
{
"id": 172,
"name": "RA",
"pretty_name": null,
"description": "J2000 coordinate",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:35:20.745194Z",
"updated": "2020-07-28T01:35:20.758294Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
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