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{
"url": "https://datacentral.org.au/api/schema/6/",
"name": "sami",
"pretty_name": "SAMI",
"title": "The SAMI Galaxy Survey",
"description": "<div id=\"project_overview_text\"><p>The SAMI Galaxy Survey is a spatially resolved spectroscopic survey of a large sample of nearby (z<0.1) galaxies, conducted with the Sydney – Australian Astronomical Observatory Multi-Object Integral Field Spectrograph (SAMI). SAMI is mounted on the 3.9 meter Anglo-Australian Telescope at Siding Spring Observatory. Survey observations began in March 2013 and were completed in May 2018. At the completion of survey observing, just over 3000 total galaxies were observed.</p><p>The key science goals of the SAMI Survey are to answer the following questions:</p><ul><li>What is the physical role of environment in galaxy evolution?</li><li>What is the relationship between stellar mass growth and angular momentum development in galaxies?</li><li>How does gas get into and out of galaxies, and how does this drive star formation?</li></ul></div>",
"pi": "Scott Croom",
"contact": {
"email": "scott.croom@sydney.edu.au",
"name": "Scott Croom"
},
"website": "http://www.sami-survey.org/",
"active": true,
"type": "Survey",
"data_releases": [
{
"name": "pdr38",
"pretty_name": "Data Release 3 (private v8)",
"version": 0.12,
"data_release_number": 3,
"contact": {
"email": "scott.croom@sydney.edu.au",
"name": "Scott Croom"
},
"created": "2020-11-30T03:13:59.251217Z",
"updated": "2020-12-14T02:45:12.820960Z",
"type": "DataRelease",
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{
"id": 38,
"name": "sami",
"pretty_name": "SAMI",
"description": "This group contains catalogue data derived from SAMI data",
"documentation": "",
"file_path": null,
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"version": "V0.12.1",
"type": "CatalogueGroup",
"created": "2020-11-30T03:14:08.924550Z",
"updated": "2020-12-09T02:22:13.726561Z",
"contact": {
"email": "scott.croom@sydney.edu.au",
"name": "Scott Croom"
},
"tables": [
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"name": "IndexAperturesDR3",
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"documentation": "<p>\nThis table contains the emission line fluxes and gas velocity and velocity dispersion determined from single Gaussian component fits to integrated SAMI spectra from a series of standard, fixed apertures. Also included are the value-added products of the extinction correction factor of the Hα line (determined from the Balmer decrement) and the Hα-based star formation rate within the aperture (assuming the SAMI standard cosmology of: H<sub>0</sub>=70 km/s, Ω<sub>m</sub>=0.3 and Ω<sub>Λ</sub>=0.7). The table includes all galaxies in the DR3 release. The standard apertures are:\n</p>\n<ol>\n <li>1.4_ARCSECOND - a 1.4 arcsecond circular aperture centred on the centre of the cube</li>\n <li>2_ARCSECOND - as above, but 2 arcseconds</li>\n <li>3_ARCSECOND - as above, but 3 arcseconds</li>\n <li>4_ARCSECOND - as above, but 4 arcseconds</li>\n <li>3KPC_ROUND - a circular aperture with a physical radius of 3kpc</li>\n <li>RE - an elliptical aperture with semi-major axis radius Re, where Re was measured using a singe-Sersic fit</li>\n <li>RE_MGE - an elliptical aperture with semi-major axis radius Re, where Re was measured using an MGE fit</li>\n</ol>\n<p>\nFor each aperture we derive the total fluxes and associated errors for:\n</p>\n<ol>\n <li>OII3726 and OII3729 - the [OII]λ3726,3729 emission line doublet (that, given their proximity, we generally recommend combining)</li>\n <li>NEIII3869 - the [NeIII]λ3869 emission line </li>\n <li>HEPSILON - the Hελ3970 emission line</li>\n <li>HDELTA - the Hδλ4102 emission line</li>\n <li>HGAMMA - the Hγλ4340 emission line</li>\n <li>OIII4363 - the [OIII]λ4363 emission line</li>\n <li>HBETA - the Hβλ4861 emission line</li>\n <li>OIII5007 - the [OIII]λ5007 emission line</li>\n <li>OI6300 - the [OI]λ5007 emission line</li>\n <li>HALPHA - the Hαλ6563 emission line</li>\n <li>NII6583 - the [NII]λ6583 emission line</li>\n <li>SII6716 and SII6731 - the [SII]λ6716 and λ6731 emission line doublet</li>\n</ol>\nwith all wavelengths given in Angstroms.\n<p>\nWhere there was insufficient signal-to-noise in a given aperture to make a reliable fit a NULL (NaN) value is recorded. For value-added products where a rel;aible estimate cannot be derived, the value or error will list a NULL or Nan value. A full description of how the measurements are derived, including the value-added products, can be found in the SAMI data release papers; <a href=\"http://adsabs.harvard.edu/abs/2018MNRAS.475..716G\">Green et al., MNRAS, 475, 716</a> and <a href=\"https://ui.adsabs.harvard.edu/abs/2018MNRAS.481.2299S\">Scott et al., 2018, MNRAS, 481, 2299</a>\n</p>\n\n",
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"created": "2020-11-30T03:14:09.298740Z",
"updated": "2020-12-09T02:22:13.977841Z",
"contact": {
"email": "brent.groves@uwa.edu.au",
"name": "Brent Groves"
},
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"name": "NII6583_1_4_ARCSECOND_ERR",
"pretty_name": null,
"description": "Uncertainty on total [NII]6583 flux in 1.4-ARCSECOND aperture",
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"contact": null,
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"id": 6890,
"name": "CUBEIDPUB",
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"description": "Public unique cube ID for data release",
"documentation": "",
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"id": 6891,
"name": "CUBEIDNAME",
"pretty_name": null,
"description": "Name of specific blue cube",
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"contact": null,
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"id": 6895,
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"pretty_name": null,
"description": "Uncertainty on Gas velocity in 1.4-ARCSECOND aperture",
"documentation": "",
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"contact": null,
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"unit": "km/s"
},
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"name": "VDISP_GAS_1_4_ARCSECOND_ERR",
"pretty_name": null,
"description": "Uncertainty on Gas velocity dispersion in 1.4-ARCSECOND aperture",
"documentation": "",
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"description": "Total [OII]3726 flux in 1.4-ARCSECOND aperture",
"documentation": "",
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"description": "Uncertainty on total [OII]3726 flux in 1.4-ARCSECOND aperture",
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},
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"description": "Uncertainty on total [OII]3729 flux in 1.4-ARCSECOND aperture",
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},
{
"id": 6904,
"name": "NEIII3869_1_4_ARCSECOND",
"pretty_name": null,
"description": "Total [NeIII]3869 flux in 1.4-ARCSECOND aperture",
"documentation": "",
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"name": "NEIII3869_1_4_ARCSECOND_ERR",
"pretty_name": null,
"description": "Uncertainty on total [NeIII]3869 flux in 1.4-ARCSECOND aperture",
"documentation": "",
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"contact": null,
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"unit": "1E-16 erg/s/cm2"
},
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"id": 6906,
"name": "HEPSILON_1_4_ARCSECOND",
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"description": "Total Hepsilon flux in 1.4-ARCSECOND aperture",
"documentation": "",
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"name": "HEPSILON_1_4_ARCSECOND_ERR",
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"description": "Uncertainty on total Hepsilon flux in 1.4-ARCSECOND aperture",
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},
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"name": "HDELTA_1_4_ARCSECOND",
"pretty_name": null,
"description": "Total Hdelta flux in 1.4-ARCSECOND aperture",
"documentation": "",
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"description": "Uncertainty on total Hdelta flux in 1.4-ARCSECOND aperture",
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"name": "HGAMMA_1_4_ARCSECOND",
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},
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},
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"description": "Total [OIII]5007 flux in 1.4-ARCSECOND aperture",
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},
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"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 6443,
"name": "CATID",
"pretty_name": null,
"description": "Object identifier",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-11-30T03:14:10.367334Z",
"updated": "2020-12-09T02:22:14.903554Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
}
]
},
{
"id": 127,
"name": "FstarCatClusters",
"pretty_name": null,
"description": "SAMI calibration stars in cluster regions",
"documentation": "<p>This table contains F-stars used for secondary flux calibration and point\nspread function measurement for SAMI Galaxy Survey observations within\nthe cluster regions. The stars with CATIDs starting with 888 are\ntaken from SDSS, while the stars starting with 999 are from VST\nATLAS. Priorities are set based on the magnitude range of the targets, with\nfainter stars having lower priority.\n</p>\n",
"file_path": "/data/ingestion_1.9/sami/pdr38/catalogues/FstarCatClusters.fits",
"file_name": "FstarCatClusters.fits",
"file_extension": "fits",
"version": "DR3",
"type": "CatalogueTable",
"created": "2020-11-30T03:14:09.099004Z",
"updated": "2020-12-09T02:22:26.765930Z",
"contact": {
"email": "matt.owers@mq.edu.au",
"name": "Matt Owers"
},
"input_cat": true,
"columns": [
{
"id": 6452,
"name": "priority",
"pretty_name": null,
"description": "Priority class for targets",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-11-30T03:14:10.618722Z",
"updated": "2020-12-09T02:22:15.053471Z",
"contact": null,
"ucd": "meta.code.class",
"unit": "-"
},
{
"id": 6450,
"name": "Dec",
"pretty_name": null,
"description": "J2000 Declination of object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-11-30T03:14:10.548469Z",
"updated": "2020-12-09T02:22:15.013145Z",
"contact": null,
"ucd": "pos.eq.dec",
"unit": "deg"
},
{
"id": 6449,
"name": "RA",
"pretty_name": null,
"description": "J2000 Right Ascension of object",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-11-30T03:14:10.528183Z",
"updated": "2020-12-09T02:22:15.001261Z",
"contact": null,
"ucd": "pos.eq.ra",
"unit": "deg"
},
{
"id": 6448,
"name": "CATID",
"pretty_name": null,
"description": "Object identifier",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-11-30T03:14:10.485997Z",
"updated": "2020-12-09T02:22:14.989016Z",
"contact": null,
"ucd": "meta.id",
"unit": "-"
},
{
"id": 6451,
"name": "r",
"pretty_name": null,
"description": "r-band PSF magnitude",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-11-30T03:14:10.565869Z",
"updated": "2020-12-09T02:22:15.033310Z",
"contact": null,
"ucd": "phot.mag",
"unit": "mag"
}
]
},
{
"id": 132,
"name": "MGEPhotomUnregDR3",
"pretty_name": null,
"description": "Results from Multi Gaussian Expansion fitting of imaging data",
"documentation": "This table contains r-band photometric properties measured from the best non-regularised Multi Gaussian Expansion of each SAMI galaxy. The full details about the measurements are available in D'Eugenio et al. (in prep.)\nThe same photometric measurements in g- and i-band are available on request.\nThe best-fit Multi Gaussian Expansion (Sigma_i, sigma_i and q_i) for each galaxy is available on request.\nRegularised measurements are available on request.\n\nThe Multi Gaussian Expansion algorithm is originally described in Emsellem et al. (1994). We used the free python implementation mgefit from Cappellari (2002).\n",
"file_path": "/data/ingestion_1.9/sami/pdr38/catalogues/MGEPhotomUnregDR3.fits",
"file_name": "MGEPhotomUnregDR3.fits",
"file_extension": "fits",
"version": "DR3",
"type": "CatalogueTable",
"created": "2020-11-30T03:14:09.229529Z",
"updated": "2020-12-09T02:22:13.920608Z",
"contact": {
"email": "francesco.deugenio@gmail.com",
"name": "Francesco D'Eugenio"
},
"input_cat": false,
"columns": [
{
"id": 6836,
"name": "Chi2",
"pretty_name": null,
"description": "Chi^2 from MGE fit.",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-11-30T03:14:25.743252Z",
"updated": "2020-12-09T02:22:21.460362Z",
"contact": null,
"ucd": "stat.fit.chi2",
"unit": "-"
},
{
"id": 6835,
"name": "dist2NNeigh",
"pretty_name&