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"created": "2020-07-28T01:37:36.009644Z",
"updated": "2020-07-28T01:37:36.023706Z",
"contact": null,
"ucd": "meta.id",
"unit": "Degrees"
},
{
"id": 3540,
"name": "RA",
"pretty_name": null,
"description": "SAMI galaxy Right Ascension",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:37:35.980799Z",
"updated": "2020-07-28T01:37:35.988287Z",
"contact": null,
"ucd": "meta.id",
"unit": "Degrees"
},
{
"id": 3539,
"name": "CATID",
"pretty_name": null,
"description": "SAMI galaxy ID",
"documentation": "",
"file_path": null,
"file_name": null,
"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:37:35.952138Z",
"updated": "2020-07-28T01:37:35.966904Z",
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}
]
},
{
"id": 74,
"name": "GasRecomcompApertures",
"pretty_name": null,
"description": "Aperture recommended-component emission line fluxes, ionised gas kinematics, and star formation rates",
"documentation": "<p>\nThis table contains measurements of fluxes, velocity and\nvelocity dispersion from the recommended multi-component Gaussian fit (1-3) for the strong 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 the total emission line fluxes and 1-sigma uncertainties for\n[OII]3727, Hβ, [OIII]5007, Hα, [NII]6583, and the\n[SII]6716,6731 doublet based on the sum of 1- to 3-component Gaussian fits. The Gaussian fits to all observed aperture spectra are made using the LZIFU fitting code (Ho et al. 2016), and the recommend number of components are determined the using a neural net (Hampton et al., 2017).\nAlso included are the Hα fluxes and determined velocities\nand velocity dispersions and 1-sigma uncertainties for the 1- to\n3-components for all apertures. When less then\n3-components are necessary, the higher-order values are left\nintentionally blank. Further value-added products included are the Balmer-line derived extinction correction and the star formation rate (if the spectra is star formation dominated) derived from the total Hα flux.\nAll measurements and fitting methods are 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",
"file_path": "/data/ingestion_1.9/sami/dr2/catalogues/sami_aperture_gas_recom_comp.fits",
"file_name": "sami_aperture_gas_recom_comp.fits",
"file_extension": "fits",
"version": "v0.10.1",
"type": "CatalogueTable",
"created": "2020-07-28T01:37:24.128327Z",
"updated": "2020-07-28T01:37:24.141495Z",
"contact": {
"email": "brent.groves@anu.edu.au",
"name": "Brent Groves"
},
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"name": "SFR_ERR_4_ARCSECOND",
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"description": "Uncertainty in star formation rate in 4-ARCSECOND aperture",
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"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:37:51.321953Z",
"updated": "2020-07-28T01:37:51.352229Z",
"contact": null,
"ucd": "phys.sfr",
"unit": "Msun/yr"
},
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"name": "SFR_4_ARCSECOND",
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"description": "Star formation rate in 4-ARCSECOND aperture",
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"type": "CatalogueColumn",
"created": "2020-07-28T01:37:51.277904Z",
"updated": "2020-07-28T01:37:51.300545Z",
"contact": null,
"ucd": "phys.sfr",
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},
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"id": 3958,
"name": "EXTINCTION_CORR_ERR_4_ARCSECOND",
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"description": "Uncertainty in extinction correction on total Halpha flux in 4-ARCSECOND apertur",
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"file_extension": null,
"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:37:51.251427Z",
"updated": "2020-07-28T01:37:51.265331Z",
"contact": null,
"ucd": "phys.fluxcorr",
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"id": 3957,
"name": "EXTINCTION_CORR_4_ARCSECOND",
"pretty_name": null,
"description": "Extinction correction on total Halpha flux in 4-ARCSECOND aperture",
"documentation": "",
"file_path": null,
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"type": "CatalogueColumn",
"created": "2020-07-28T01:37:51.208210Z",
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"name": "SII6731_ERR_4_ARCSECOND",
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"version": null,
"type": "CatalogueColumn",
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"updated": "2020-07-28T01:37:51.195185Z",
"contact": null,
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"unit": "1E-16 erg/s/cm2"
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"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:37:51.146298Z",
"updated": "2020-07-28T01:37:51.160214Z",
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"name": "SII6716_ERR_4_ARCSECOND",
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"type": "CatalogueColumn",
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"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:37:51.020822Z",
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"name": "NII6583_4_ARCSECOND",
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"documentation": "",
"file_path": null,
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"type": "CatalogueColumn",
"created": "2020-07-28T01:37:50.987454Z",
"updated": "2020-07-28T01:37:51.000375Z",
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"type": "CatalogueColumn",
"created": "2020-07-28T01:37:50.962003Z",
"updated": "2020-07-28T01:37:50.975281Z",
"contact": null,
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},
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"id": 3949,
"name": "HALPHA_3_COMP_4_ARCSECOND",
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"description": "3-component Halpha flux in 4-ARCSECOND aperture",
"documentation": "",
"file_path": null,
"file_name": null,
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"version": null,
"type": "CatalogueColumn",
"created": "2020-07-28T01:37:50.937173Z",
"updated": "2020-07-28T01:37:50.942292Z",
"contact": null,
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"version": null,
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"updated": "2020-07-28T01:37:50.916998Z",
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"version": null,
"type": "CatalogueColumn",
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"contact": null,
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},
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"name": "HALPHA_1_COMP_4_ARCSECOND",
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"description": "1-component Halpha flux in 4-ARCSECOND aperture",
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"type": "CatalogueColumn",
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"created": "2020-07-28T01:37:50.759642Z",
"updated": "2020-07-28T01:37:50.772571Z",
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},
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"description": "Uncertainty on total [OI]6300 flux in 4-ARCSECOND aperture",
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