Table Description:
This table is available for ADQL queries and through the TAP endpoint.
Resource Description:
For a list of all services and tables belonging to this table's resource, see Information on resource 'ASPIC GAMA'
To cite the table as such, we suggest the following BibTeX entry:
![[Operator logo]](/static/img/logo_medium.png){kind=logo}
@MISC{vo:aspic_gama_g09g1,
year=2021,
title={{ASPIC} {GAMA}},
author={Baldry et al. and Pipien et al. and {ASPIC} team},
url={https://vo.lam.fr/tableinfo/aspic_gama.g09g12g15},
howpublished={{VO} resource provided by the {CeSAM} Virtual Observatory Server}
}
GAMA (Galaxy And Mass Assembly) [1] is a joint European-Australasian project based on spectroscopic observations using the AAOmega multi-object spectrograph on the Anglo-Australian Telescope (AAT).
This resource contains the ASPIC [2] value added catalogues on a selection of GAMA DR3 sources. To the GAMA DR3 photometry - Baldry et al. 2018 (2018MNRAS.474.3875B) and Liske et al. 2015 (2015MNRAS.452.2087L) - the ASPIC team added physical properties computed with Le Phare [3] and CIGALE [4] using the GAZPAR [5] service, as well as line informations obtained by processing the GAMA spectra with the Slinefit software (Schreiber et al., 2018 - 2018A&A...618A..85S).
The GAMA information is coming from G02TilingCat, SpecAll, and G02CFHTLSInputCat in G02InputCat(v07). The GAMA spectral features are coming from GaussFitComplex in SpecLineSFR (v05).
To this, the ASPIC team added MAG_AUTO magnitudes for GALEX (~5600 objects), WIRCam Ks (~14000 objects, LAM observations), and LAM WIRCam Y-band magnitudes described in Pipien et al. 2018 (2018A&A...616A..55P). These magnitudes were added by cross-matching the catalogues with a 1 arc-second radius.
Only the sources with a NQ quality better or equal to 2, CFHTLS magnitudes in all the bands, and a reliable Y-band were kept, resulting in a catalogue of almost 32000 objects.
The GAMA information is coming from SpecAll in SpecCat (v27), ApMatchedCat in ApMatchedPhotom (v06), GaussFitComplex in SpecLineSFR (v05), and MagPhys (v06).
Only the sources with a NQ quality better or equal to 2 and reliable measurements in all the bands were kept, resulting in a catalogue of about 119000 objects.
ASPIC (Archives Spectrophotométriques Publiques Intégrées au CeSAM) is the public spectro-photometric archive of the Laboratoire d'Astrophysique de Marseille data-centre (CeSAM, Centre de donnéeS Astrophysiques de Marseille). We give access to spectro-photometric data with value additions like physical parameters, photometric redshifts, and spectra line measurements.
GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programmes including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/.
If your paper makes use of GAMA data products based on VISTA VIKING data, please also include the following: Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 179.A-2004.
If your paper makes use of GAMA data products based on VST KiDS data, please also include the following: Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 177.A-3016.
Research work benefiting from the use of ASPIC data at CeSAM should include the following acknowledgement in publications: “This research has made use of the ASPIC database, operated at CeSAM/LAM, Marseille, France.”
| [1] | http://www.gama-survey.org/ |
| [2] | Archives Spectrophotométriques Publiques Intégrées au CeSAM, https://cesam.lam.fr/aspic |
| [3] | https://cesam.lam.fr/lephare |
| [4] | https://cigale.lam.fr |
| [5] | https://gazpar.lam.fr |
Sorted alphabetically. [Sort by DB column index]
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| abs_fei_3582_errew | abs_FeI_3582_errEW | Uncertainty on SLINEFIT FeI equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_fei_3582_errflux | abs_FeI_3582_errflux | Uncertainty on SLINEFIT FeI measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_fei_3582_errfluxbkg | abs_FeI_3582_errfluxbkg | Uncertainty on SLINEFIT FeI background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_fei_3582_ew | abs_FeI_3582_EW | SLINEFIT FeI equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_fei_3582_flux | abs_FeI_3582_flux | SLINEFIT FeI measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_fei_3582_fluxbkg | abs_FeI_3582_fluxbkg | SLINEFIT FeI background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_feii_2344_errew | abs_FeII_2344_errEW | Uncertainty on SLINEFIT FeII 2344 equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_feii_2344_errflux | abs_FeII_2344_errflux | Uncertainty on SLINEFIT FeII 2344 measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_feii_2344_errfluxbkg | abs_FeII_2344_errfluxbkg | Uncertainty on SLINEFIT FeII 2344 background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_feii_2344_ew | abs_FeII_2344_EW | SLINEFIT FeII 2344 equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_feii_2344_flux | abs_FeII_2344_flux | SLINEFIT FeII 2344 measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_feii_2344_fluxbkg | abs_FeII_2344_fluxbkg | SLINEFIT FeII 2344 background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_feii_2380_1_errew | abs_FeII_2380_1_errEW | Uncertainty on SLINEFIT FeII 2380_1 equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_feii_2380_1_errflux | abs_FeII_2380_1_errflux | Uncertainty on SLINEFIT FeII 2380_1 measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_feii_2380_1_errfluxbkg | abs_FeII_2380_1_errfluxbkg | Uncertainty on SLINEFIT FeII 2380_1 background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_feii_2380_1_ew | abs_FeII_2380_1_EW | SLINEFIT FeII 2380_1 equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_feii_2380_1_flux | abs_FeII_2380_1_flux | SLINEFIT FeII 2380_1 measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_feii_2380_1_fluxbkg | abs_FeII_2380_1_fluxbkg | SLINEFIT FeII 2380_1 background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_feii_2380_2_errew | abs_FeII_2380_2_errEW | Uncertainty on SLINEFIT FeII 2380_2 equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_feii_2380_2_errflux | abs_FeII_2380_2_errflux | Uncertainty on SLINEFIT FeII 2380_2 measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_feii_2380_2_errfluxbkg | abs_FeII_2380_2_errfluxbkg | Uncertainty on SLINEFIT FeII 2380_2 background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_feii_2380_2_ew | abs_FeII_2380_2_EW | SLINEFIT FeII 2380_2 equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_feii_2380_2_flux | abs_FeII_2380_2_flux | SLINEFIT FeII 2380_2 measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_feii_2380_2_fluxbkg | abs_FeII_2380_2_fluxbkg | SLINEFIT FeII 2380_2 background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_feii_2600_1_errew | abs_FeII_2600_1_errEW | Uncertainty on SLINEFIT FeII 2600_1 equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_feii_2600_1_errflux | abs_FeII_2600_1_errflux | Uncertainty on SLINEFIT FeII 2600_1 measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_feii_2600_1_errfluxbkg | abs_FeII_2600_1_errfluxbkg | Uncertainty on SLINEFIT FeII 2600_1 background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_feii_2600_1_ew | abs_FeII_2600_1_EW | SLINEFIT FeII 2600_1 equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_feii_2600_1_flux | abs_FeII_2600_1_flux | SLINEFIT FeII 2600_1 measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_feii_2600_1_fluxbkg | abs_FeII_2600_1_fluxbkg | SLINEFIT FeII 2600_1 background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_feii_2600_2_errew | abs_FeII_2600_2_errEW | Uncertainty on SLINEFIT FeII 2600_2 equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_feii_2600_2_errflux | abs_FeII_2600_2_errflux | Uncertainty on SLINEFIT FeII 2600_2 measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_feii_2600_2_errfluxbkg | abs_FeII_2600_2_errfluxbkg | Uncertainty on SLINEFIT FeII 2600_2 background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_feii_2600_2_ew | abs_FeII_2600_2_EW | SLINEFIT FeII 2600_2 equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_feii_2600_2_flux | abs_FeII_2600_2_flux | SLINEFIT FeII 2600_2 measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_feii_2600_2_fluxbkg | abs_FeII_2600_2_fluxbkg | SLINEFIT FeII 2600_2 background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_gband_4304_errew | abs_Gband_4304_errEW | Uncertainty on SLINEFIT Gband equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_gband_4304_errflux | abs_Gband_4304_errflux | Uncertainty on SLINEFIT Gband measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_gband_4304_errfluxbkg | abs_Gband_4304_errfluxbkg | Uncertainty on SLINEFIT Gband background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_gband_4304_ew | abs_Gband_4304_EW | SLINEFIT Gband equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_gband_4304_flux | abs_Gband_4304_flux | SLINEFIT Gband measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_gband_4304_fluxbkg | abs_Gband_4304_fluxbkg | SLINEFIT Gband background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_h_3969_errew | abs_H_3969_errew | Uncertainty on SLINEFIT H equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_h_3969_errflux | abs_H_3969_errflux | Uncertainty on SLINEFIT H measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_h_3969_errfluxbkg | abs_H_3969_errfluxbkg | Uncertainty on SLINEFIT H background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_h_3969_ew | abs_H_3969_ew | SLINEFIT H equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_h_3969_flux | abs_H_3969_flux | SLINEFIT H measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_h_3969_fluxbkg | abs_H_3969_fluxbkg | SLINEFIT H background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_halpha_6564_errew | abs_Halpha_6564_errEW | Uncertainty on SLINEFIT Halpha equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line.Halpha |
| abs_halpha_6564_errflux | abs_Halpha_6564_errflux | Uncertainty on SLINEFIT Halpha measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Halpha |
| abs_halpha_6564_errfluxbkg | abs_Halpha_6564_errfluxbkg | Uncertainty on SLINEFIT Halpha background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Halpha;instr.background |
| abs_halpha_6564_ew | abs_Halpha_6564_EW | SLINEFIT Halpha equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line.Halpha |
| abs_halpha_6564_flux | abs_Halpha_6564_flux | SLINEFIT Halpha measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Halpha |
| abs_halpha_6564_fluxbkg | abs_Halpha_6564_fluxbkg | SLINEFIT Halpha background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Halpha;instr.background |
| abs_hbeta_4862_errew | abs_Hbeta_4862_errEW | Uncertainty on SLINEFIT Hbeta equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line.Hbeta |
| abs_hbeta_4862_errflux | abs_Hbeta_4862_errflux | Uncertainty on SLINEFIT Hbeta measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hbeta |
| abs_hbeta_4862_errfluxbkg | abs_Hbeta_4862_errfluxbkg | Uncertainty on SLINEFIT Hbeta background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hbeta;instr.background |
| abs_hbeta_4862_ew | abs_Hbeta_4862_EW | SLINEFIT Hbeta equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line.Hbeta |
| abs_hbeta_4862_flux | abs_Hbeta_4862_flux | SLINEFIT Hbeta measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Hbeta |
| abs_hbeta_4862_fluxbkg | abs_Hbeta_4862_fluxbkg | SLINEFIT Hbeta background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Hbeta;instr.background |
| abs_hdelta_4102_errew | abs_Hdelta_4102_errEW | Uncertainty on SLINEFIT Hdelta equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line.Hdelta |
| abs_hdelta_4102_errflux | abs_Hdelta_4102_errflux | Uncertainty on SLINEFIT Hdelta measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hdelta |
| abs_hdelta_4102_errfluxbkg | abs_Hdelta_4102_errfluxbkg | Uncertainty on SLINEFIT Hdelta background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hdelta;instr.background |
| abs_hdelta_4102_ew | abs_Hdelta_4102_EW | SLINEFIT Hdelta equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line.Hdelta |
| abs_hdelta_4102_flux | abs_Hdelta_4102_flux | SLINEFIT Hdelta measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Hdelta |
| abs_hdelta_4102_fluxbkg | abs_Hdelta_4102_fluxbkg | SLINEFIT Hdelta background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Hdelta;instr.background |
| abs_hgamma_4341_errew | abs_Hgamma_4341_errEW | Uncertainty on SLINEFIT Hgamma equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line.Hgamma |
| abs_hgamma_4341_errflux | abs_Hgamma_4341_errflux | Uncertainty on SLINEFIT Hgamma measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hgamma |
| abs_hgamma_4341_errfluxbkg | abs_Hgamma_4341_errfluxbkg | Uncertainty on SLINEFIT Hgamma background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hgamma;instr.background |
| abs_hgamma_4341_ew | abs_Hgamma_4341_EW | SLINEFIT Hgamma equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line.Hgamma |
| abs_hgamma_4341_flux | abs_Hgamma_4341_flux | SLINEFIT Hgamma measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Hgamma |
| abs_hgamma_4341_fluxbkg | abs_Hgamma_4341_fluxbkg | SLINEFIT Hgamma background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line.Hgamma;instr.background |
| abs_k_3934_errew | abs_K_3934_errEW | Uncertainty on SLINEFIT K equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_k_3934_errflux | abs_K_3934_errflux | Uncertainty on SLINEFIT K measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_k_3934_errfluxbkg | abs_K_3934_errfluxbkg | Uncertainty on SLINEFIT K background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_k_3934_ew | abs_K_3934_EW | SLINEFIT K equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_k_3934_flux | abs_K_3934_flux | SLINEFIT K measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_k_3934_fluxbkg | abs_K_3934_fluxbkg | SLINEFIT K background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_mgi_5176_errew | abs_MgI_5176_errEW | Uncertainty on SLINEFIT MgI equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_mgi_5176_errflux | abs_MgI_5176_errflux | Uncertainty on SLINEFIT MgI measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_mgi_5176_errfluxbkg | abs_MgI_5176_errfluxbkg | Uncertainty on SLINEFIT MgI background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_mgi_5176_ew | abs_MgI_5176_EW | SLINEFIT MgI equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_mgi_5176_flux | abs_MgI_5176_flux | SLINEFIT MgI measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_mgi_5176_fluxbkg | abs_MgI_5176_fluxbkg | SLINEFIT MgI background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_mgii_2797_errew | abs_MgII_2797_errEW | Uncertainty on SLINEFIT MgII 2797 equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_mgii_2797_errflux | abs_MgII_2797_errflux | Uncertainty on SLINEFIT MgII 2797 measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_mgii_2797_errfluxbkg | abs_MgII_2797_errfluxbkg | Uncertainty on SLINEFIT MgII 2797 background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_mgii_2797_ew | abs_MgII_2797_EW | SLINEFIT MgII 2797 equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_mgii_2797_flux | abs_MgII_2797_flux | SLINEFIT MgII 2797 measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_mgii_2797_fluxbkg | abs_MgII_2797_fluxbkg | SLINEFIT MgII 2797 background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_mgii_2804_errew | abs_MgII_2804_errEW | Uncertainty on SLINEFIT MgII 2804 equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_mgii_2804_errflux | abs_MgII_2804_errflux | Uncertainty on SLINEFIT MgII 2804 measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_mgii_2804_errfluxbkg | abs_MgII_2804_errfluxbkg | Uncertainty on SLINEFIT MgII 2804 background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_mgii_2804_ew | abs_MgII_2804_EW | SLINEFIT MgII 2804 equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_mgii_2804_flux | abs_MgII_2804_flux | SLINEFIT MgII 2804 measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_mgii_2804_fluxbkg | abs_MgII_2804_fluxbkg | SLINEFIT MgII 2804 background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| abs_nad_5895_errew | abs_NaD_5895_errEW | Uncertainty on SLINEFIT NaD equivalent width in absorption | Angstrom | stat.error;spect.line.eqWidth;em.line |
| abs_nad_5895_errflux | abs_NaD_5895_errflux | Uncertainty on SLINEFIT NaD measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| abs_nad_5895_errfluxbkg | abs_NaD_5895_errfluxbkg | Uncertainty on SLINEFIT NaD background flux measure in absorption | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| abs_nad_5895_ew | abs_NaD_5895_EW | SLINEFIT NaD equivalent width in absorption | Angstrom | spect.line.eqWidth;em.line |
| abs_nad_5895_flux | abs_NaD_5895_flux | SLINEFIT NaD measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line |
| abs_nad_5895_fluxbkg | abs_NaD_5895_fluxbkg | SLINEFIT NaD background flux measure in absorption | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| agem_percentile50 | agem_percentile50 | Median mass-weighted age (GAMA, MAGPHYS) | log(yr) | stat.fit;stat.median;time.age |
| ager_percentile50 | ager_percentile50 | Median r-band light-weighted age (GAMA, MAGPHYS) | log(yr) | stat.fit;stat.median;time.age |
| cataid | CataId | GAMA DR3 unique identifier | N/A | meta.id;meta.main |
| cig_fracagn | cig_fracAGN | Dust luminosity AGN fraction fitted by CIGALE | N/A | stat.fit.param;arith.ratio;meta.modelled |
| cig_lir | cig_LIR | Infrared luminosity fitted with CIGALE with AGN component | log(W) | stat.fit;phys.luminosity;em.ir;meta.modelled |
| cig_mstar | cig_mStar | Stellar mass fitted with CIGALE with AGN component | log(solMass) | stat.fit;phys.mass;meta.modelled |
| cig_noagn_lir | cig_noAGN_LIR | Infrared luminosity fitted with CIGALE without AGN component | log(W) | stat.fit;phys.luminosity;em.ir;meta.modelled |
| cig_noagn_mstar | cig_noAGN_mStar | Stellar mass fitted with CIGALE without AGN component | log(solMass) | stat.fit;phys.mass;meta.modelled |
| cig_noagn_sfr | cig_noAGN_SFR | Star Formation Rate fitted with CIGALE without AGN component | log(solMass/yr) | stat.fit;phys.sfr;meta.modelled |
| cig_sfr | cig_SFR | Star Formation Rate fitted with CIGALE with AGN component | log(solMass/yr) | stat.fit;phys.sfr;meta.modelled |
| dec | Dec | Declination | deg | pos.eq.dec;meta.main |
| e_cig_fracagn | e_cig_fracAGN | Uncertainty on cig_fracAGN | N/A | stat.error;stat.fit.param;arith.ratio;meta.modelled |
| e_cig_lir | e_cig_LIR | Uncertainty on cig_LIR | log(W) | stat.error;stat.fit;phys.luminosity;em.ir;meta.modelled |
| e_cig_mstar | e_cig_mStar | Uncertainty on cig_mStar | log(solMass) | stat.error;stat.fit;phys.mass;meta.modelled |
| e_cig_noagn_lir | e_cig_noAGN_LIR | Uncertainty on cig_noAGN_LIR | log(W) | stat.error;stat.fit;phys.luminosity;em.ir;meta.modelled |
| e_cig_noagn_mstar | e_cig_noAGN_mStar | Uncertainty on cig_noAGN_mStar | log(solMass) | stat.error;stat.fit;phys.mass;meta.modelled |
| e_cig_noagn_sfr | e_cig_noAGN_SFR | Uncertainty on cig_noAGN_SFR | log(solMass/yr) | stat.error;stat.fit;phys.sfr;meta.modelled |
| e_cig_sfr | e_cig_SFR | Uncertainty on cig_SFR | log(solMass/yr) | stat.error;stat.fit;phys.sfr;meta.modelled |
| e_galex_fuv | e_GALEX_FUV | Uncertainty on GALEX_FUV | uJy | stat.error;phot.flux.density;em.uv.100-200nm |
| e_galex_nuv | e_GALEX_NUV | Uncertainty on GALEX_NUV | uJy | stat.error;phot.flux.density;em.uv.200-300nm |
| e_gama_ha_b_ew | e_GAMA_Ha_B_EW | uncertainty on GAMA_Ha_B_EW | Angstrom | stat.error;spect.line.eqWidth;em.line.Halpha |
| e_gama_ha_b_flux | e_GAMA_Ha_B_flux | Uncertainty on GAMA_Ha_B_flux | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | stat.error;phot.flux;em.line.Halpha |
| e_gama_ha_ew | e_GAMA_Ha_EW | Uncertainty on GAMA_Ha_EW | Angstrom | stat.error;spect.line.eqWidth;em.line.Halpha |
| e_gama_ha_flux | e_GAMA_Ha_flux | Uncertainty on GAMA_Ha_flux | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | stat.error;phot.flux;em.line.Halpha |
| e_gama_hb_b_ew | e_GAMA_Hb_B_EW | Uncertainty on GAMA_Hb_B_EW | Angstrom | stat.error;spect.line.eqWidth;em.line.Hbeta |
| e_gama_hb_b_flux | e_GAMA_Hb_B_flux | Uncertainty on GAMA_Hb_B_flux | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | stat.error;phot.flux;em.line.Hbeta |
| e_gama_hb_ew | e_GAMA_Hb_EW | Uncertainty on GAMA_Hb_EW | Angstrom | stat.error;spect.line.eqWidth;em.line.Hbeta |
| e_gama_hb_flux | e_gama_Hb_flux | Uncertainty on GAMA_Hb_flux | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | stat.error;phot.flux;em.line.Hbeta |
| e_gama_niia_ew | e_GAMA_NIIa_ew | Uncertainty on GAMA_NIIa_EW | Angstrom | stat.error;spect.line.eqWidth;em.line |
| e_gama_niia_flux | e_GAMA_NIIa_flux | Uncertainty on GAMA_NIIa_flux | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | stat.error;phot.flux;em.line |
| e_gama_niib_ew | e_GAMA_NIIb_ew | Uncertainty on GAMA_NIIb_EW | Angstrom | stat.error;spect.line.eqWidth;em.line |
| e_gama_niib_flux | e_GAMA_NIIb_flux | Uncertainty on GAMA_NIIb_flux | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | stat.error;phot.flux;em.line |
| e_gama_oiiia_ew | e_GAMA_OIIIa_EW | Uncertainty on GAMA_OIIIa_EW | Angstrom | stat.error;spect.line.eqWidth;em.line.OIII |
| e_gama_oiiia_flux | e_GAMA_OIIIa_flux | Uncertainty on GAMA_OIIIa_flux | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line.OIII |
| e_pacs_100 | e_PACS_100 | Uncertainty on PACS_100 | mJy | stat.error;phot.flux.density;em.ir.60-100um |
| e_pacs_160 | e_PACS_160 | Uncertainty on PACS_160 | mJy | stat.error;phot.flux.density;em.mm.1500-3000ghz |
| e_sdss_g | e_SDSS_g | Uncertainty on SDSS_g | mag | stat.error;phot.mag;em.opt.B |
| e_sdss_i | e_SDSS_i | Uncertainty on SDSS_i | mag | stat.error;phot.mag;em.opt.R |
| e_sdss_r | e_SDSS_r | Uncertainty SDSS_r | mag | stat.error;phot.mag;em.opt.R |
| e_sdss_u | e_SDSS_u | Uncertainty SDSS_u | mag | stat.error;phot.mag;em.opt.U |
| e_sdss_z | e_SDSS_z | Uncertainty on SDSS_z | mag | stat.error;phot.mag;em.opt.I |
| e_spire_250 | e_SPIRE_250 | Uncertainty on SPIRE_250 | mJy | stat.error;phot.flux.density;em.mm.750-1500ghz |
| e_spire_350 | e_SPIRE_350 | Uncertainty on SPIRE_350 | mJy | stat.error;phot.flux.density;em.mm.750-1500ghz |
| e_spire_500 | e_SPIRE_500 | Uncertainty on SPIRE_500 | mJy | stat.error;phot.flux.density;em.mm.400-750ghz |
| e_vista_h | e_VISTA_H | Uncertainty on VISTA_H | mag | stat.error;phot.mag;em.IR.H |
| e_vista_j | e_VISTA_J | Uncertainty on VISTA_J | mag | stat.error;phot.mag;em.IR.J |
| e_vista_ks | e_VISTA_Ks | Uncertainty on VISTA_Ks | mag | stat.error;phot.mag;em.IR.K |
| e_vista_y | e_VISTA_Y | Uncertainty on VISTA_Y | mag | stat.error;phot.mag;em.IR.J |
| e_vista_z | e_VISTA_Z | Uncertainty on VISTA_Z | mag | stat.error;phot.mag;em.opt.I |
| e_wise_w1 | e_WISE_W1 | Uncertainty on WISE_W1 | mJy | stat.error;phot.flux.density;em.IR.3-4um |
| e_wise_w2 | e_WISE_W2 | Uncertainty on WISE_W2 | mJy | stat.error;phot.flux.density;em.IR.4-8um |
| e_wise_w3 | e_WISE_W3 | Uncertainty on WISE_W3 | mJy | stat.error;phot.flux.density;em.IR.8-15um |
| e_wise_w4 | e_WISE_W4 | Uncertainty on WISE_W4 | mJy | stat.error;phot.flux.density;em.IR.15-30um |
| em_ciii_1908_errew | em_CIII_1908_errEW | Uncertainty on SLINEFIT CIII equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_ciii_1908_errflux | em_CIII_1908_errflux | Uncertainty on SLINEFIT CIII measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_ciii_1908_errfluxbkg | em_CIII_1908_errfluxbkg | Uncertainty on SLINEFIT CIII background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_ciii_1908_ew | em_CIII_1908_EW | SLINEFIT CIII equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_ciii_1908_flux | em_CIII_1908_flux | SLINEFIT CIII measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_ciii_1908_fluxbkg | em_CIII_1908_fluxbkg | SLINEFIT CIII background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_halpha_errew | em_Halpha_errEW | Uncertainty on SLINEFIT Halpha equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line.Halpha |
| em_halpha_errflux | em_Halpha_errflux | Uncertainty on SLINEFIT Halpha measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Halpha |
| em_halpha_errfluxbkg | em_Halpha_errfluxbkg | Uncertainty on SLINEFIT Halpha background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Halpha;instr.background |
| em_halpha_ew | em_Halpha_EW | SLINEFIT Halpha equivalent width in emission | Angstrom | spect.line.eqWidth;em.line.Halpha |
| em_halpha_flux | em_Halpha_flux | SLINEFIT Halpha measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Halpha |
| em_halpha_fluxbkg | em_Halpha_fluxbkg | SLINEFIT Halpha background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Halpha;instr.background |
| em_hbeta_errew | em_Hbeta_errEW | Uncertainty on SLINEFIT Hbeta equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line.Hbeta |
| em_hbeta_errflux | em_Hbeta_errflux | Uncertainty on SLINEFIT Hbeta measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hbeta |
| em_hbeta_errfluxbkg | em_Hbeta_errfluxbkg | Uncertainty on SLINEFIT Hbeta background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hbeta;instr.background |
| em_hbeta_ew | em_Hbeta_EW | SLINEFIT Hbeta equivalent width in emission | Angstrom | spect.line.eqWidth;em.line.Hbeta |
| em_hbeta_flux | em_Hbeta_flux | SLINEFIT Hbeta measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Hbeta |
| em_hbeta_fluxbkg | em_Hbeta_fluxbkg | SLINEFIT Hbeta background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Hbeta;instr.background |
| em_hdelta_errew | em_Hdelta_errEW | Uncertainty on SLINEFIT Hdelta equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line.Hdelta |
| em_hdelta_errflux | em_Hdelta_errflux | Uncertainty on SLINEFIT Hdelta measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hdelta |
| em_hdelta_errfluxbkg | em_Hdelta_errfluxbkg | Uncertainty on SLINEFIT Hdelta background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hdelta;instr.background |
| em_hdelta_ew | em_Hdelta_EW | SLINEFIT Hdelta equivalent width in emission | Angstrom | spect.line.eqWidth;em.line.Hdelta |
| em_hdelta_flux | em_Hdelta_flux | SLINEFIT Hdelta measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Hdelta |
| em_hdelta_fluxbkg | em_Hdelta_fluxbkg | SLINEFIT Hdelta background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Hdelta;instr.background |
| em_hgamma_errew | em_Hgamma_errEW | Uncertainty on SLINEFIT Hgamma equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line.Hgamma |
| em_hgamma_errflux | em_Hgamma_errflux | Uncertainty on SLINEFIT Hgamma measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hgamma |
| em_hgamma_errfluxbkg | em_Hgamma_errfluxbkg | Uncertainty on SLINEFIT Hgamma background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.Hgamma;instr.background |
| em_hgamma_ew | em_Hgamma_EW | SLINEFIT Hgamma equivalent width in emission | Angstrom | spect.line.eqWidth;em.line.Hgamma |
| em_hgamma_flux | em_Hgamma_flux | SLINEFIT Hgamma measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Hgamma |
| em_hgamma_fluxbkg | em_Hgamma_fluxbkg | SLINEFIT Hgamma background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.Hgamma;instr.background |
| em_mgii_2799_errew | em_MgII_2799_errEW | Uncertainty on SLINEFIT MgII 2799 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_mgii_2799_errflux | em_MgII_2799_errflux | Uncertainty on SLINEFIT MgII 2799 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_mgii_2799_errfluxbkg | em_MgII_2799_errfluxbkg | Uncertainty on SLINEFIT MgII 2799 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_mgii_2799_ew | em_MgII_2799_EW | SLINEFIT MgII 2799 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_mgii_2799_flux | em_MgII_2799_flux | SLINEFIT MgII 2799 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_mgii_2799_fluxbkg | em_MgII_2799_fluxbkg | SLINEFIT MgII 2799 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_nii_6549_errew | em_NII_6549_errEW | Uncertainty on SLINEFIT NII 6549 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_nii_6549_errflux | em_NII_6549_errflux | Uncertainty on SLINEFIT NII 6549 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_nii_6549_errfluxbkg | em_NII_6549_errfluxbkg | Uncertainty on SLINEFIT NII 6549 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_nii_6549_ew | em_NII_6549_EW | SLINEFIT NII 6549 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_nii_6549_flux | em_NII_6549_flux | SLINEFIT NII 6549 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_nii_6549_fluxbkg | em_NII_6549_fluxbkg | SLINEFIT NII 6549 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_nii_6583_1_errew | em_NII_6583_1_errEW | Uncertainty on SLINEFIT NII_1 6583 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_nii_6583_1_errflux | em_NII_6583_1_errflux | Uncertainty on SLINEFIT NII_1 6583 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_nii_6583_1_errfluxbkg | em_NII_6583_1_errfluxbkg | Uncertainty on SLINEFIT NII_1 6583 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_nii_6583_1_ew | em_NII_6583_1_EW | SLINEFIT NII_1 6583 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_nii_6583_1_flux | em_NII_6583_1_flux | SLINEFIT NII_1 6583 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_nii_6583_1_fluxbkg | em_NII_6583_1_fluxbkg | SLINEFIT NII_1 6583 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_nii_6583_2_errew | em_NII_6583_2_errEW | Uncertainty on SLINEFIT NII_2 6583 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_nii_6583_2_errflux | em_NII_6583_2_errflux | Uncertainty on SLINEFIT NII_2 6583 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_nii_6583_2_errfluxbkg | em_NII_6583_2_errfluxbkg | Uncertainty on SLINEFIT NII_2 6583 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_nii_6583_2_ew | em_NII_6583_2_EW | SLINEFIT NII_2 6583 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_nii_6583_2_flux | em_NII_6583_2_flux | SLINEFIT NII_2 6583 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_nii_6583_2_fluxbkg | em_NII_6583_2_fluxbkg | SLINEFIT NII_2 6583 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_oii_3727_1_errew | em_OII_3727_1_errEW | Uncertainty on SLINEFIT OII_1 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_oii_3727_1_errflux | em_OII_3727_1_errflux | Uncertainty on SLINEFIT OII_1 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_oii_3727_1_errfluxbkg | em_OII_3727_1_errfluxbkg | Uncertainty on SLINEFIT OII_1 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_oii_3727_1_ew | em_OII_3727_1_EW | SLINEFIT OII_1 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_oii_3727_1_flux | em_OII_3727_1_flux | SLINEFIT OII_1 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_oii_3727_1_fluxbkg | em_OII_3727_1_fluxbkg | SLINEFIT OII_1 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_oii_3727_2_errew | em_02_3727_2_errEW | Uncertainty on SLINEFIT OII_2 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_oii_3727_2_errflux | em_OII_3727_2_errflux | Uncertainty on SLINEFIT OII_2 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_oii_3727_2_errfluxbkg | em_OII_3727_2_errfluxbkg | Uncertainty on SLINEFIT OII_2 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_oii_3727_2_ew | em_OII_3727_2_EW | SLINEFIT OII_2 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_oii_3727_2_flux | em_OII_3727_2_flux | SLINEFIT OII_2 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_oii_3727_2_fluxbkg | em_OII_3727_2_fluxbkg | SLINEFIT OII_2 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_oiii_5007_1_errew | em_OIII_5007_1_errEW | Uncertainty on SLINEFIT OIII_1 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line.OIII |
| em_oiii_5007_1_errflux | em_OIII_5007_1_errflux | Uncertainty on SLINEFIT OIII_1 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.OIII |
| em_oiii_5007_1_errfluxbkg | em_OIII_5007_1_errfluxbkg | Uncertainty on SLINEFIT OIII_1 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.OIII;instr.background |
| em_oiii_5007_1_ew | em_OIII_5007_1_EW | SLINEFIT OIII_1 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line.OIII |
| em_oiii_5007_1_flux | em_OIII_5007_1_flux | SLINEFIT OIII_1 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.OIII |
| em_oiii_5007_1_fluxbkg | em_OIII_5007_1_fluxbkg | SLINEFIT OIII_1 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.OIII;instr.background |
| em_oiii_5007_2_errew | em_OIII_5007_2_errEW | Uncertainty on SLINEFIT OIII_2 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line.OIII |
| em_oiii_5007_2_errflux | em_OIII_5007_2_errflux | Uncertainty on SLINEFIT OIII_2 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.OIII |
| em_oiii_5007_2_errfluxbkg | em_OIII_5007_2_errfluxbkg | Uncertainty on SLINEFIT OIII_2 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line.OIII;instr.background |
| em_oiii_5007_2_ew | em_OIII_5007_2_EW | SLINEFIT OIII_2 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line.OIII |
| em_oiii_5007_2_flux | em_OIII_5007_2_flux | SLINEFIT OIII_2 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.OIII |
| em_oiii_5007_2_fluxbkg | em_OIII_5007_2_fluxbkg | SLINEFIT OIII_2 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line.OIII;instr.background |
| em_sii_6718_errew | em_SII_6718_errEW | Uncertainty on SLINEFIT SII 6718 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_sii_6718_errflux | em_SII_6718_errflux | Uncertainty on SLINEFIT SII 6718 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_sii_6718_errfluxbkg | em_SII_6718_errfluxbkg | Uncertainty on SLINEFIT SII 6718 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_sii_6718_ew | em_SII_6718_EW | SLINEFIT SII 6718 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_sii_6718_flux | em_SII_6718_flux | SLINEFIT SII 6718 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_sii_6718_fluxbkg | em_SII_6718_fluxbkg | SLINEFIT SII 6718 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| em_sii_6732_errew | em_SII_6732_errEW | Uncertainty on SLINEFIT SII 6732 equivalent width in emission | Angstrom | stat.error;spect.line.eqWidth;em.line |
| em_sii_6732_errflux | em_SII_6732_errflux | Uncertainty on SLINEFIT SII 6732 measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line |
| em_sii_6732_errfluxbkg | em_SII_6732_errfluxbkg | Uncertainty on SLINEFIT SII 6732 background flux measure in emission | erg.cm**-2.s**-1 | stat.error;phot.flux;em.line;instr.background |
| em_sii_6732_ew | em_SII_6732_EW | SLINEFIT SII 6732 equivalent width in emission | Angstrom | spect.line.eqWidth;em.line |
| em_sii_6732_flux | em_SII_6732_flux | SLINEFIT SII 6732 measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line |
| em_sii_6732_fluxbkg | em_SII_6732_fluxbkg | SLINEFIT SII 6732 background flux measure in emission | erg.cm**-2.s**-1 | phot.flux;em.line;instr.background |
| f_mu_ir_best_fit | f_mu_IR_best_fit | Best fit fraction of L_sun accounted by dust in the ambient ISM (GAMA, MAGPHYS) | N/A | stat.fit;phys.absorption.opticalDepth;em.opt.V |
| f_mu_ir_percentile50 | f_mu_IR_percentile50 | Median fraction of L_sun accounted by dust in the ambient ISM (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.absorption.opticalDepth;em.opt.V |
| f_mu_sfh_best_fit | f_mu_SFH_best_fit | Best fit fraction of tau_V^BC contributed by dust in the HII region (GAMA, MAGPHYS) | N/A | stat.fit;phys.absorption.opticalDepth;em.opt.V |
| f_mu_sfh_percentile50 | f_mu_SFH_percentile50 | Median fraction of tau_V^BC contributed by dust in the HII region (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.absorption.opticalDepth;em.opt.V |
| fb17_percentile50 | fb17_percentile50 | Median fraction of stellar mass formed in bursts over last 10^7 yr (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.mass |
| fb19_percentile50 | fb19_percentile50 | Median fraction of stellar mass formed in bursts over last 10^9 yr (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.mass |
| galex_fuv | GALEX_FUV | GALEX FUV flux (GAMA) | uJy | phot.flux.density;em.uv.100-200nm |
| galex_nuv | GALEX_NUV | GALEX NUV flux (GAMA) | uJy | phot.flux.density;em.uv.200-300nm |
| gama_ha_b_ew | GAMA_Ha_B_EW | GAMA equivalent width for the broad component of Hα in emission | Angstrom | spect.line.eqWidth;em.line.Halpha |
| gama_ha_b_flux | GAMA_Ha_B_flux | GAMA flux for the broad component of Hα in emission (the unit is valid only for SDSS and AAOmega spectra) | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line.Halpha |
| gama_ha_ew | GAMA_Ha_EW | GAMA equivalent width for Hα in emission | Angstrom | spect.line.eqWidth;em.line.Halpha |
| gama_ha_flux | GAMA_Ha_flux | GAMA flux for Hα in emission (the unit is valid only for SDSS and AAOmega spectra) | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line.Halpha |
| gama_hb_b_ew | GAMA_Hb_B_EW | GAMA equivalent width for the broad component of Hβ in emission | Angstrom | spect.line.eqWidth;em.line.Hbeta |
| gama_hb_b_flux | GAMA_Hb_B_flux | GAMA flux for the broad component of Hβ in emission (the unit is valid only for SDSS and AAOmega spectra) | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line.Hbeta |
| gama_hb_ew | GAMA_Hb_EW | GAMA equivalent width for Hβ in emission | Angstrom | spect.line.eqWidth;em.line.Hbeta |
| gama_hb_flux | GAMA_Hb_flux | GAMA flux for Hβ in emission (the unit is valid only for SDSS and AAOmega spectra) | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line.Hbeta |
| gama_niia_ew | GAMA_NIIa_EW | GAMA equivalent width for the strong (red) component of [NII] | Angstrom | spect.line.eqWidth;em.line |
| gama_niia_flux | GAMA_NIIa_flux | GAMA flux for the strong (red) component of [NII] (the unit is valid only for SDSS and AAOmega spectra) | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line |
| gama_niib_ew | GAMA_NIIb_EW | GAMA equivalent width for the weak (blue) component of [NII] | Angstrom | spect.line.eqWidth;em.line |
| gama_niib_flux | GAMA_NIIb_flux | GAMA flux for the weak (blue) component of [NII] (the unit is valid only for SDSS and AAOmega spectra) | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line |
| gama_oiiia_ew | GAMA_OIIIa_EW | GAMA equivalent width for the strong (red) component of [OIII] | Angstrom | spect.line.eqWidth;em.line.OIII |
| gama_oiiia_flux | GAMA_OIIIa_flux | GAMA flux for the strong (red) component of [OIII] (the unit is valid only for SDSS and AAOmega spectra) | 1e-17erg.s**-1.cm**-2.Angstrom**-1 | phot.flux;em.line.OIII |
| gamma_percentile50 | gamma_percentile50 | Median star formation timescale (GAMA, MAGPHYS) | Gyr**-1 | stat.fit;stat.median;phys.SFR;time.scale |
| l_dust_best_fit | L_dust_best_fit | Best fit total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM, GAMA, MAGPHYS) | solLum | stat.fit;phys.luminosity |
| l_dust_percentile50 | L_dust_percentile50 | Median total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM, GAMA, MAGPHYS) | log(solLum) | stat.fit;stat.median;phys.luminosity |
| lp_age | lp_age | Median age from the analysis (LePhare) | yr | time.age;stat.fit;stat.median;meta.modelled |
| lp_age_inf | lp_age_inf | Age 16% lower value from the analysis (LePhare) | yr | time.age;stat.fit;stat.min;meta.modelled |
| lp_age_sup | lp_age_sup | Age 16% higher value from the analysis (LePhare) | yr | time.age;stat.fit;stat.max;meta.modelled |
| lp_sfr | lp_SFR | Median log Star Formation Rate from the analysis (LePhare) | log(solMass/yr) | phys.SFR;stat.fit;stat.median;meta.modelled |
| lp_sfr_inf | lp_SFR_inf | Log Star Formation Rate lower 16% value from the analysis (LePhare) | log(solMass/yr) | phys.SFR;stat.fit;stat.min;meta.modelled |
| lp_sfr_sup | lp_SFR_sup | Log Star Formation Rate higher 16% value from the analysis (LePhare) | log(solMass/yr) | phys.SFR;stat.fit;stat.max;meta.modelled |
| lp_ssfr | lp_sSFR | Median log specific Star Formation Rate from the analysis (LePhare) | log(yr**-1) | phys.SFR;stat.fit;stat.median;meta.modelled |
| lp_ssfr_inf | lp_sSFR_inf | Log specific Star Formation Rate lower 16% value from the analysis (LePhare) | log(yr**-1) | phys.SFR;stat.fit;stat.min;meta.modelled |
| lp_ssfr_sup | lp_sSFR_sup | Log specific Star Formation Rate higher 16% value from the analysis (LePhare) | log(yr**-1) | phys.SFR;stat.fit;stat.max;meta.modelled |
| lp_stellar_mass | lp_stellar_mass | Median log stellar mass from the analysis (LePhare) | log(solMass) | phys.mass;stat.fit;stat.median;meta.modelled |
| lp_stellar_mass_inf | lp_stellar_mass_inf | Log stellar mass 16% lower value from the analysis (LePhare) | log(solMass) | phys.mass;stat.fit;stat.min;meta.modelled |
| lp_stellar_mass_sup | lp_stellar_mass_sup | Log stellar mass 16% higher value from the analysis (LePhare) | log(solMass) | phys.mass;stat.fit;stat.max;meta.modelled |
| mabs_galex_fuv | mAbs_GALEX_FUV | Absolute GALEX FUV AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.uv.100-200nm;stat.fit;meta.modelled |
| mabs_galex_nuv | mAbs_GALEX_NUV | Absolute GALEX NUV AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.uv.200-300nm;stat.fit;meta.modelled |
| mabs_pacs_100 | mAbs_PACS_100 | Absolute Herschel PACS 100µm AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.ir.60-100um;stat.fit;meta.modelled |
| mabs_pacs_160 | mAbs_PACS_160 | Absolute Herschel PACS 160µm AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.mm.1500-3000ghz;stat.fit;meta.modelled |
| mabs_sdss_g | mAbs_SDSS_g | Absolute SDSS g AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.opt.B;stat.fit;meta.modelled |
| mabs_sdss_i | mAbs_SDSS_i | Absolute SDSS i AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.opt.I;stat.fit;meta.modelled |
| mabs_sdss_r | mAbs_SDSS_r | Absolute SDSS r AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.opt.R;stat.fit;meta.modelled |
| mabs_sdss_u | mAbs_SDSS_u | Absolute SDSS u AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.opt.U;stat.fit;meta.modelled |
| mabs_sdss_z | mAbs_SDSS_z | Absolute SDSS z AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.opt.I;stat.fit;meta.modelled |
| mabs_spire_250 | mAbs_SPIRE_250 | Absolute Herschel SPIRE 250µm AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.mm.750-1500ghz;stat.fit;meta.modelled |
| mabs_spire_350 | mAbs_SPIRE_350 | Absolute Herschel SPIRE 350µm AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.mm.750-1500ghz;stat.fit;meta.modelled |
| mabs_spire_500 | mAbs_SPIRE_500 | Absolute Herschel SPIRE 500µm AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.mm.400-750ghz;stat.fit;meta.modelled |
| mabs_vista_h | mAbs_VISTA_H | Absolute VISTA H AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.IR.H;stat.fit;meta.modelled |
| mabs_vista_j | mAbs_VISTA_J | Absolute VISTA J AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.IR.J;stat.fit;meta.modelled |
| mabs_vista_ks | mAbs_VISTA_Ks | Absolute VISTA Ks AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.IR.K;stat.fit;meta.modelled |
| mabs_vista_y | mAbs_VISTA_Y | Absolute VISTA Y AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.IR.J;stat.fit;meta.modelled |
| mabs_vista_z | mAbs_VISTA_Z | Absolute VISTA Z AB magnitude from the analysis (LePhare) | mag | phys.magAbs;em.opt.I;stat.fit;meta.modelled |
| mass_dust_best_fit | mass_dust_best_fit | Best fit total mass of dust (GAMA, MAGPHYS) | solMass | stat.fit;phys.mass |
| mass_dust_percentile50 | mass_dust_percentile50 | Median total mass of dust (GAMA, MAGPHYS) | log(solMass) | stat.fit;stat.median;phys.mass |
| mass_stellar_best_fit | mass_stellar_best_fit | Best fit total mass of stars ever formed; integral of the star formation rate (GAMA, MAGPHYS) | solMass | stat.fit;phys.mass |
| mass_stellar_percentile50 | mass_stellar_percentile50 | Median total mass of stars ever formed; integral of the star formation rate (GAMA, MAGPHYS) | log(solMass) | stat.fit;stat.median;phys.mass |
| metalicity_z_zo_percentile50 | metalicity_Z_Zo_percentile50 | Median metallicity in solar units (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.abund.Z |
| mu_parameter_best_fit | mu_parameter_best_fit | Best fit fraction of tau_V contributed by dust in the ambient ISM (GAMA, MAGPHYS) | N/A | stat.fit;phys.absorption.opticalDepth;em.opt.V |
| mu_parameter_percentile50 | mu_parameter_percentile50 | Median fraction of tau_V contributed by dust in the ambient ISM (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.absorption.opticalDepth;em.opt.V |
| pacs_100 | PACS_100 | Herschel PACS 100µm flux (GAMA) | mJy | phot.flux.density;em.ir.60-100um |
| pacs_160 | PACS_160 | Herschel PACS 160µm flux (GAMA) | mJy | phot.flux.density;em.mm.1500-3000ghz |
| ra | RA | Right Ascension | deg | pos.eq.ra;meta.main |
| sdss_g | SDSS_g | SDSS g Kron AB magnitude (GAMA) | mag | phot.mag;em.opt.B |
| sdss_i | SDSS_i | SDSS i Kron AB magnitude (GAMA) | mag | phot.mag;em.opt.I |
| sdss_r | SDSS_r | SDSS r Kron AB magnitude (GAMA) | mag | phot.mag;em.opt.R |
| sdss_u | SDSS_u | SDSS u Kron AB magnitude (GAMA) | mag | phot.mag;em.opt.U |
| sdss_z | SDSS_z | SDSS z Kron AB magnitude (GAMA) | mag | phot.mag;em.opt.I |
| sfr17_percentile50 | sfr17_percentile50 | Median star-formation rate averaged over the last 10^7 yr (GAMA, MAGPHYS) | log(solMass/yr) | stat.fit;stat.median;phys.SFR |
| sfr19_percentile50 | sfr19_percentile50 | Median star-formation rate averaged over the last 10^9 yr (GAMA, MAGPHYS) | log(solMass/yr) | stat.fit;stat.median;phys.SFR |
| sfr_0_1gyr_best_fit | SFR_0_1Gyr_best_fit | Best fit star formation rate (GAMA, MAGPHYS) | solMass/yr | stat.fit;phys.SFR |
| sfr_0_1gyr_percentile50 | SFR_0_1Gyr_percentile50 | Median star formation rate (GAMA, MAGPHYS) | log(solMass/yr) | stat.fit;stat.median;phys.SFR |
| spectrum_accref | Spectrum_accref | Access key to the associated GAMA DR3 spectrum | N/A | meta.id |
| spire_250 | SPIRE_250 | Herschel SPIRE 250µm flux (GAMA) | mJy | phot.flux.density;em.mm.750-1500ghz |
| spire_350 | SPIRE_350 | Herschel SPIRE 350µm flux (GAMA) | mJy | phot.flux.density;em.mm.750-1500ghz |
| spire_500 | SPIRE_500 | Herschel SPIRE 500µm flux (GAMA) | mJy | phot.flux.density;em.mm.400-750ghz |
| ssfr_0_1gyr_best_fit | sSFR_0_1Gyr_best_fit | Best fit specific star formation rate (GAMA, MAGPHYS) | yr**-1 | stat.fit;phys.SFR |
| ssfr_0_1gyr_percentile50 | sSFR_0_1Gyr_percentile50 | Median of specific star formation rate (GAMA, MAGPHYS) | log(yr**-1) | stat.fit;stat.median;phys.SFR |
| t_c_ism_best_fit | T_C_ISM_best_fit | Best fit equilibrium temperature of cold dust in the ambient ISM (GAMA, MAGPHYS) | K | stat.fit;phys.temperature |
| t_c_ism_percentile50 | T_C_ISM_percentile50 | Median equilibrium temperature of cold dust in the ambient ISM (GAMA, MAGPHYS) | K | stat.fit;stat.median;phys.temperature |
| t_w_bc_best_fit | T_W_BC_best_fit | Best fit equilibrium temperature of warm dust in the ambient ISM (GAMA, MAGPHYS) | K | stat.fit;phys.temperature |
| t_w_bc_percentile50 | T_W_BC_percentile50 | Median equilibrium temperature of warm dust in the ambient ISM (GAMA, MAGPHYS) | K | stat.fit;stat.median;phys.temperature |
| tau_v_best_fit | tau_V_best_fit | Best fit total V-band optical depth of the dust seen by young stars in their birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;phys.absorption.opticalDepth;em.opt.V |
| tau_v_ism_best_fit | tau_V_ISM_best_fit | Best fit total V-band optical depth of the dust seen through the ISM (GAMA, MAGPHYS) | N/A | stat.fit;phys.absorption.opticalDepth;em.opt.V |
| tau_v_ism_percentile50 | tau_V_ISM_percentile50 | Median total V-band optical depth of the dust seen through the ISM (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.absorption.opticalDepth;em.opt.V |
| tau_v_percentile50 | tau_V_percentile50 | Median total V-band optical depth of the dust seen by young stars in their birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.absorption.opticalDepth;em.opt.V |
| tform_percentile50 | tform_percentile50 | Median age of the oldest stars in the galaxy (GAMA, MAGPHYS) | log(yr) | stat.fit;stat.median;time.age |
| tlastb_percentile50 | tlastb_percentile50 | Median time since the last burst of star formation ended (GAMA, MAGPHYS) | log(yr) | stat.fit;stat.median;time.age |
| vista_h | VISTA_H | VIKING VISTA VIRCAM H Kron AB magnitude (GAMA) | mag | phot.mag;em.IR.H |
| vista_j | VISTA_J | VIKING VISTA VIRCAM J Kron AB magnitude (GAMA) | mag | phot.mag;em.IR.J |
| vista_ks | VISTA_Ks | VIKING VISTA VIRCAM Ks Kron AB magnitude (GAMA) | mag | phot.mag;em.IR.K |
| vista_y | VISTA_Y | VIKING VISTA VIRCAM Y Kron AB magnitude (GAMA) | mag | phot.mag;em.IR.J |
| vista_z | VISTA_Z | VIKING VISTA VIRCAM Z Kron AB magnitude (GAMA) | mag | phot.mag;em.opt.I |
| wise_w1 | WISE_W1 | WISE W1 flux (GAMA) | mJy | phot.flux.density;em.IR.3-4um |
| wise_w2 | WISE_W2 | WISE W2 flux (GAMA) | mJy | phot.flux.density;em.IR.4-8um |
| wise_w3 | WISE_W3 | WISE W3 flux (GAMA) | mJy | phot.flux.density;em.IR.8-15um |
| wise_w4 | WISE_W4 | WISE W4 flux (GAMA) | mJy | phot.flux.density;em.IR.15-30um |
| xi_c_tot_best_fit | xi_C_tot_best_fit | Best fit fractional contribution by cold dust to the dust luminosity of the ambient ISM (GAMA, MAGPHYS) | N/A | stat.fit;phys.luminosity |
| xi_c_tot_percentile50 | xi_C_tot_percentile50 | Median fractional contribution by cold dust to the dust luminosity of the ambient ISM (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.luminosity |
| xi_mir_tot_best_fit | xi_MIR_tot_best_fit | Best fit fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;phys.luminosity |
| xi_mir_tot_percentile50 | xi_MIR_tot_percentile50 | Median fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.luminosity |
| xi_pah_tot_best_fit | xi_PAH_tot_best_fit | Best fit fractional contribution by PAHs to the dust luminosity of the stellar birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;phys.luminosity |
| xi_pah_tot_percentile50 | xi_PAH_tot_percentile50 | Median fractional contribution by PAHs to the dust luminosity of the stellar birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.luminosity |
| xi_w_tot_best_fit | xi_W_tot_best_fit | Best fit fractional contribution by warm dust to the dust luminosity of the stellar birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;phys.luminosity |
| xi_w_tot_percentile50 | xi_W_tot_percentile50 | Median fractional contribution by warm dust to the dust luminosity of the stellar birth clouds (GAMA, MAGPHYS) | N/A | stat.fit;stat.median;phys.luminosity |
| z | z | Spectroscopic redshift | N/A | src.redshift |
Columns that are parts of indices are marked like this.
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