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"updated": "2022-07-12T03:29:32.832373Z",
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"id": 13734,
"name": "VDISP_GAS_ERR_2_COMP_RE",
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"updated": "2022-07-12T03:29:32.775069Z",
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"updated": "2022-07-12T03:29:32.726747Z",
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"description": "Uncertainty on 1-component Gas velocity dispersion in RE aperture",
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"updated": "2022-07-12T03:29:32.708208Z",
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"description": "1-component Gas velocity dispersion in RE aperture",
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"updated": "2022-07-12T03:29:32.671244Z",
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"name": "V_GAS_3_COMP_ERR_RE",
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"description": "Uncertainty on 3-component Gas velocity in RE aperture",
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"name": "V_GAS_2_COMP_ERR_RE",
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"description": "Uncertainty on 2-component Gas velocity in RE aperture",
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"updated": "2022-07-12T03:29:32.572768Z",
"contact": null,
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},
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"id": 13727,
"name": "V_GAS_2_COMP_RE",
"pretty_name": null,
"description": "2-component Gas velocity in RE aperture",
"documentation": "",
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"created": "2022-07-12T03:29:32.546240Z",
"updated": "2022-07-12T03:29:32.552392Z",
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"id": 13726,
"name": "V_GAS_1_COMP_ERR_RE",
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"description": "Uncertainty on 1-component Gas velocity in RE aperture",
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"updated": "2022-07-12T03:29:32.533240Z",
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"id": 13725,
"name": "V_GAS_1_COMP_RE",
"pretty_name": null,
"description": "1-component Gas velocity in RE aperture",
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"updated": "2022-07-12T03:29:32.514489Z",
"contact": null,
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},
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"id": 13724,
"name": "AREA_COV_RE",
"pretty_name": null,
"description": "Fraction of SAMI FoV covered by RE aperture",
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"name": "NPIX_RE",
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"description": "Number of pixels in RE aperture",
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"version": null,
"type": "CatalogueColumn",
"created": "2022-07-12T03:29:32.456713Z",
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"id": 13722,
"name": "PA",
"pretty_name": null,
"description": "SAMI galaxy Position Angle",
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"created": "2022-07-12T03:29:32.410362Z",
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"contact": null,
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},
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"id": 13721,
"name": "ELLIP",
"pretty_name": null,
"description": "SAMI galaxy ellipticity",
"documentation": "",
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"type": "CatalogueColumn",
"created": "2022-07-12T03:29:32.378291Z",
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"id": 13720,
"name": "R_E",
"pretty_name": null,
"description": "SAMI galaxy effective radius",
"documentation": "",
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"type": "CatalogueColumn",
"created": "2022-07-12T03:29:32.344700Z",
"updated": "2022-07-12T03:29:32.357721Z",
"contact": null,
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"id": 13719,
"name": "Z",
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"description": "SAMI galaxy Redshift assumed",
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"updated": "2022-07-12T03:29:32.324363Z",
"contact": null,
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"id": 13718,
"name": "DEC",
"pretty_name": null,
"description": "SAMI galaxy Declination",
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"version": null,
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"created": "2022-07-12T03:29:32.292908Z",
"updated": "2022-07-12T03:29:32.297648Z",
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"id": 13717,
"name": "RA",
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"contact": null,
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},
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"id": 13716,
"name": "CATAID",
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"description": "SAMI galaxy ID",
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"id": 273,
"name": "Gas1compApertures",
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"description": "Aperture 1-component emission line fluxes, ionised gas kinematics, and star formation rates",
"documentation": "<p>\nThis table contains measurements of the fluxes, velocity and\nvelocity dispersion measured using a single Gaussian fit to the strong ionised-gas optical emission lines in a series of standard, fixed apertures. It includes all galaxies in the Data Release 2 sample. The measurements are performed on the v0.10.1 SAMI DR2 aperture spectra. The standard apertures are:\n</p>\n<ul style=\"list-style-type:disc\">\n<li>1.4_ARCSECOND - a 1.4 arc second circular aperture centred on the centre of the cube</li>\n<li>2_ARCSECOND - as above, but 2 arc seconds</li>\n<li>3_ARCSECOND - as above, but 3 arc seconds</li>\n<li>4_ARCSECOND - as above, but 4 arc seconds</li>\n<li>3_KPC_ROUND - a circular aperture with a physical radius of 3kpc</li>\n<li>RE - an elliptical aperture with semi-major axis of radius Re</li>\n</ul>\n<p>\nThe table includes emission line fluxes for\n[OII]3727, Hβ, [OIII]5007, Hα, [NII]6583, and the\n[SII]6716,6731 doublet determined using a 1-component Gaussian fit, as\nwell as the determined velocity and velocity dispersion and associated\n1-sigma uncertainties. Further value-added products included are the Balmer-line derived extinction correction and the star formation rate (if the spectra is star formation dominated). The measurements are determined from fits to the observed aperture spectra using the LZIFU fitting code (Ho et al. 2016), and fully described in Scott et al., 2017, MNRAS, 472, 2833 (http://adsabs.harvard.edu/abs/2017MNRAS.472.2833S). Note, however, that the apertures are different from the measurements in that paper, so although the technique is identical, the values for a given galaxy may not be.\n</p>\n<p>\nWhere the no lines exist or if a fit does not satisfying our quality criteria, a value of NaN is recorded (see Scott et al. (2018) for details).\n</p>\n",
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"created": "2022-07-12T03:29:18.906728Z",
"updated": "2022-07-12T03:29:18.917464Z",
"contact": {
"email": "brent.groves@anu.edu.au",
"name": "Brent Groves"
},
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"name": "SFR_ERR_4_ARCSECOND",
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"description": "Total [SII]6731 flux in the 4 arcsecond aperture",
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"description": "Uncertainty on total [NII]6583 flux in the 4 arcsecond aperture",
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},
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"id": 13705,
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"description": "Uncertainty on 1-component Halpha flux in the 4 arcsecond aperture",
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"description": "1-component Halpha flux in the 4 arcsecond aperture",
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"created": "2022-07-12T03:29:31.880835Z",
"updated": "2022-07-12T03:29:31.886207Z",
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},
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"id": 13701,
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"description": "Uncertainty on total [OI]6300 flux in the 4 arcsecond aperture",
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"description": "Total [OI]6300 flux in the 4 arcsecond aperture",
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},
{
"id": 13699,
"name": "OIII5007_ERR_4_ARCSECOND",
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"description": "Uncertainty on total [OIII]5007 flux in the 4 arcsecond aperture",
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