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Find detailed descriptions of the data available in each data release

The Schema Browser displays an extensive explanation of each type of data product each
survey/archive offers,
along with any relevant analysis and publication information (see also individual survey
documentation for more info).
For more information on the schema browser, go to the Schema Browser Documentation.
For more information on the data products within the schema browser, go to the team's documentation
on Data
Central (the link for each survey can be found in the `Meta` box below).

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.

At the heart of this project lies the GAMA spectroscopic survey of ~300,000 galaxies down to r < 19.8 mag over ~286 deg^{2}, carried out using the AAOmega multi-object spectrograph on the Anglo-Australian Telescope (AAT) by the GAMA team. 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 Sloan Digital Sky Survey (SDSS), the 2dF Galaxy Redshift Survey(2dFGRS) and the Millennium Galaxy Catalogue (MGC).

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This DMU provides k-corrections in the GALEX FUV and NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands for all GAMA DR2 galaxies.

This table provides k-corrections at redshift 0.0 in the GALEX FUV and NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands for all GAMA DR2 galaxies.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z_TONRY | - | Flow corrected redshift using Tonry et al. model | src.redshift |

Z_MODEL_ERR | mag | SDSS DR6 z-band model magnitude error | stat.error;phot.mag;em.opt.I |

Z_MODEL | mag | SDSS DR6 z-band model magnitude | phot.mag;em.opt.I |

U_MODEL_ERR | mag | SDSS DR6 u-band model magnitude error | stat.error;phot.mag;em.opt.U |

U_MODEL | mag | SDSS DR6 u-band model magnitude | phot.mag;em.opt.U |

R_MODEL_ERR | mag | SDSS DR6 r-band model magnitude error | stat.error;phot.mag;em.opt.R |

R_MODEL | mag | SDSS DR6 r-band model magnitude | phot.mag;em.opt.R |

PCOEFF_Z_5 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_4 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_3 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_2 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_1 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Y_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_U_5 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_4 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_3 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_2 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_1 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_R_5 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_4 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_3 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_2 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_1 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_NUV_5 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_4 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_3 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_2 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_1 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_K_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_J_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_I_5 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_4 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_3 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_2 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_1 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_H_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_G_5 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_4 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_3 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_2 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_1 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_FUV_5 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_4 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_3 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_2 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_1 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

NQ | - | Redshift quality | meta.code.qual;src.redshift |

METS | - | Average metallicity of currently surviving stars | phys.abund.Z |

MASS | M_solar | Stellar mass of currently surviving stars | phys.mass |

KCORR_Z | mag | K-correction in SDSS z band | phot.mag;em.opt.Z |

KCORR_Y | mag | K-correction in UKIDSS Y band | phot.mag;em.IR.NIR |

KCORR_U | mag | K-correction in SDSS u band | phot.mag;em.opt.U |

KCORR_R | mag | K-correction in SDSS r band | phot.mag;em.opt.R |

KCORR_NUV | mag | K-correction in GALEX NUV band | phot.mag;em.UV.200-300nm |

KCORR_K | mag | K-correction in UKIDSS K band | phot.mag;em.IR.K |

KCORR_J | mag | K-correction in UKIDSS J band | phot.mag;em.IR.J |

KCORR_I | mag | K-correction in SDSS i band | phot.mag;em.opt.I |

KCORR_H | mag | K-correction in UKIDSS H band | phot.mag;em.IR.H |

KCORR_G | mag | K-correction in SDSS g band | phot.mag;em.opt.G |

KCORR_FUV | mag | K-correction in GALEX FUV band | phot.mag;em.UV.100-200nm |

I_MODEL_ERR | mag | SDSS DR6 i-band model magnitude error | stat.error;phot.mag;em.opt.I |

I_MODEL | mag | SDSS DR6 i-band model magnitude | phot.mag;em.opt.I |

INTSFH | - | Total integrated star-formation history (number of stars formed total) | meta.number |

G_MODEL_ERR | mag | SDSS DR6 g-band model magnitude error | stat.error;phot.mag;em.opt.B |

G_MODEL | mag | SDSS DR6 g-band model magnitude | phot.mag;em.opt.B |

COEFFS_5 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_4 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_3 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_2 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_1 | - | kcorrect eigenspectra coefficient | arith.factor |

CHI2 | - | Chi^2 of fit returned by kcorrect | stat.fit.chi2 |

CATAID | - | Unique GAMA ID | meta.id;meta.main |

B300 | - | Fraction of the total star formation that has occurred in the last 0.3 Gyr | arith.ratio |

B1000 | - | Fraction of the total star formation that has occurred in the last 1 Gyr | arith.ratio |

This table provides k-corrections at redshift 0.1 in the GALEX FUV and NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands for all GAMA DR2 galaxies.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z_TONRY | - | Flow corrected redshift using Tonry et al. model | src.redshift |

Z_MODEL_ERR | mag | SDSS DR6 z-band model magnitude error | stat.error;phot.mag;em.opt.I |

Z_MODEL | mag | SDSS DR6 z-band model magnitude | phot.mag;em.opt.I |

U_MODEL_ERR | mag | SDSS DR6 u-band model magnitude error | stat.error;phot.mag;em.opt.U |

U_MODEL | mag | SDSS DR6 u-band model magnitude | phot.mag;em.opt.U |

R_MODEL_ERR | mag | SDSS DR6 r-band model magnitude error | stat.error;phot.mag;em.opt.R |

R_MODEL | mag | SDSS DR6 r-band model magnitude | phot.mag;em.opt.R |

PCOEFF_Z_5 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_4 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_3 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_2 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Z_1 | - | Coefficient of polynomial fit to K(z) in SDSS z band | arith.factor |

PCOEFF_Y_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_Y_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS Y band | arith.factor |

PCOEFF_U_5 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_4 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_3 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_2 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_U_1 | - | Coefficient of polynomial fit to K(z) in SDSS u band | arith.factor |

PCOEFF_R_5 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_4 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_3 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_2 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_R_1 | - | Coefficient of polynomial fit to K(z) in SDSS r band | arith.factor |

PCOEFF_NUV_5 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_4 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_3 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_2 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_NUV_1 | - | Coefficient of polynomial fit to K(z) in GALEX NUV band | arith.factor |

PCOEFF_K_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_K_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS K band | arith.factor |

PCOEFF_J_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_J_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS J band | arith.factor |

PCOEFF_I_5 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_4 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_3 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_2 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_I_1 | - | Coefficient of polynomial fit to K(z) in SDSS i band | arith.factor |

PCOEFF_H_5 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_4 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_3 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_2 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_H_1 | - | Coefficient of polynomial fit to K(z) in UKIDSS H band | arith.factor |

PCOEFF_G_5 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_4 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_3 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_2 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_G_1 | - | Coefficient of polynomial fit to K(z) in SDSS g band | arith.factor |

PCOEFF_FUV_5 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_4 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_3 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_2 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

PCOEFF_FUV_1 | - | Coefficient of polynomial fit to K(z) in GALEX FUV band | arith.factor |

NQ | - | Redshift quality | meta.code.qual;src.redshift |

METS | - | Average metallicity of currently surviving stars | phys.abund.Z |

MASS | M_solar | Stellar mass of currently surviving stars | phys.mass |

KCORR_Z | mag | K-correction in SDSS z band | phot.mag;em.opt.Z |

KCORR_Y | mag | K-correction in UKIDSS Y band | phot.mag;em.IR.NIR |

KCORR_U | mag | K-correction in SDSS u band | phot.mag;em.opt.U |

KCORR_R | mag | K-correction in SDSS r band | phot.mag;em.opt.R |

KCORR_NUV | mag | K-correction in GALEX NUV band | phot.mag;em.UV.200-300nm |

KCORR_K | mag | K-correction in UKIDSS K band | phot.mag;em.IR.K |

KCORR_J | mag | K-correction in UKIDSS J band | phot.mag;em.IR.J |

KCORR_I | mag | K-correction in SDSS i band | phot.mag;em.opt.I |

KCORR_H | mag | K-correction in UKIDSS H band | phot.mag;em.IR.H |

KCORR_G | mag | K-correction in SDSS g band | phot.mag;em.opt.G |

KCORR_FUV | mag | K-correction in GALEX FUV band | phot.mag;em.UV.100-200nm |

I_MODEL_ERR | mag | SDSS DR6 i-band model magnitude error | stat.error;phot.mag;em.opt.I |

I_MODEL | mag | SDSS DR6 i-band model magnitude | phot.mag;em.opt.I |

INTSFH | - | Total integrated star-formation history (number of stars formed total) | meta.number |

G_MODEL_ERR | mag | SDSS DR6 g-band model magnitude error | stat.error;phot.mag;em.opt.B |

G_MODEL | mag | SDSS DR6 g-band model magnitude | phot.mag;em.opt.B |

COEFFS_5 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_4 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_3 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_2 | - | kcorrect eigenspectra coefficient | arith.factor |

COEFFS_1 | - | kcorrect eigenspectra coefficient | arith.factor |

CHI2 | - | Chi^2 of fit returned by kcorrect | stat.fit.chi2 |

CATAID | - | Unique GAMA ID | meta.id;meta.main |

B300 | - | Fraction of the total star formation that has occurred in the last 0.3 Gyr | arith.ratio |

B1000 | - | Fraction of the total star formation that has occurred in the last 1 Gyr | arith.ratio |

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This DMU provides stellar masses, restframe photometry, and other ancillary stellar population parameters for all z < 0.65 galaxies in the GAMA DR2 sample.

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This table provides stellar masses, restframe photometry, and other ancillary stellar population parameters from stellar population fits to ugriz SEDs for all z < 0.65 galaxies in the GAMA DR2 sample.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

zmax_19p8 | - | Maximum redshift for which r_petro <= 19.8 (G12 SURVEY_CLASS>=6 selection) | src.redshift;stat.max |

zmax_19p4 | - | Maximum redshift for which r_petro <= 19.4 (G09/G15 SURVEY_CLASS>=6 selection) | src.redshift;stat.max |

zmax_17p88 | - | Maximum redshift for which r_petro <= 17.8 (SDSS main survey selection) | src.redshift;stat.max |

uminusr_stars | mag | Intrinsic, stellar (u-r) colour from SED fit, i.e. corrected for internal dust obscuration | phot.color |

uminusr | mag | Restframe (u-r) colour from SED fit | phot.color |

nbands | - | Number of bands used in SPS fits (max. is 5; NIR data have not been used) | meta.number |

nQ | - | Normalised redshift quality (use nQ > 2 for science) | meta.code.qual;src.redshift |

metal | - | SPS stellar metallicity (Z_Sol = 0.02) | phys.abund.Z |

logtau | dex | SPS e-folding time for the exponentially declining SFH, represented as log10(tau/[yr]) | time.scale |

logmstar | dex | Stellar mass within the photometric aperture represented as log10(M_*/[M_Sol]) (see notes) | phys.mass |

logmoverl_i | dex | Mass-to-light ratio (restframe i-band) represented as log10( (M_*/L_i) / [M_Sol/L_Sol,i] ) | phys.composition.massLightRatio |

logage | dex | SPS age T = t(z_obs) - t(z_form), represented as log10(T/[yr]) | time.age |

logLWage | dex | Restframe i-band luminosity weighted mean stellar age, represented as log10(t*/[yr]) | time.age |

gminusi_stars | mag | Intrinsic, stellar (g-i) colour from SED fit, i.e. corrected for internal dust obscuration | phot.color |

gminusi | mag | Restframe (g-i) colour from SED fit | phot.color |

fluxscale | - | Aperture correction factor for scaling total luminosities and stellar masses (see notes) | arith.factor |

fitphot_z | mag | Best-fit observers` frame z-band apparent magnitude from SPS SED fits | phot.mag |

fitphot_u | mag | Best-fit observers` frame u-band apparent magnitude from SPS SED fits | phot.mag |

fitphot_r | mag | Best-fit observers` frame r-band apparent magnitude from SPS SED fits | phot.mag |

fitphot_i | mag | Best-fit observers` frame i-band apparent magnitude from SPS SED fits | phot.mag |

fitphot_g | mag | Best-fit observers` frame g-band apparent magnitude from SPS SED fits | phot.mag |

extBV | mag | SPS dust obscuration; for Calzetti et al. (2003) dust A_V = 3.1 x E(B-V) | phys.absorption |

deluminusr | mag | Formal uncertainty on uminusr | stat.error |

delmetal | - | Formal uncertainty on metal | stat.error |

dellogtau | dex | Formal uncertainty on logtau | stat.error |

dellogmstar | dex | Formal uncertainty on logmstar | stat.error |

dellogmoverl_i | dex | Formal uncertainty on logmoverl_i | stat.error |

dellogage | dex | Formal uncertainty on logage | stat.error |

dellogLWage | dex | Formal uncertainty on logLWage | stat.error |

delgminusi | mag | Formal uncertainty on gminusi | stat.error |

delfitphot_z | mag | Formal uncertainty in fitphot_z | stat.error |

delfitphot_u | mag | Formal uncertainty in fitphot_u | stat.error |

delfitphot_r | mag | Formal uncertainty in fitphot_r | stat.error |

delfitphot_i | mag | Formal uncertainty in fitphot_i | stat.error |

delfitphot_g | mag | Formal uncertainty in fitphot_g | stat.error |

delextBV | mag | Formal uncertainty on extBV | stat.error |

delabsmag_z | mag | Formal uncertainty in absmag_z | stat.error |

delabsmag_u | mag | Formal uncertainty in absmag_u | stat.error |

delabsmag_r | mag | Formal uncertainty in absmag_r | stat.error |

delabsmag_i | mag | Formal uncertainty in absmag_i | stat.error |

delabsmag_g | mag | Formal uncertainty in absmag_g | stat.error |

absmag_z_stars | mag | Intrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe z-band | phys.magAbs |

absmag_z | mag | Absolute magnitude in restframe z-band from SPS SED fits | phys.magAbs |

absmag_u_stars | mag | Intrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe u-band | phys.magAbs |

absmag_u | mag | Absolute magnitude in restframe u-band from SPS SED fits | phys.magAbs |

absmag_r_stars | mag | Intrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe r-band | phys.magAbs |

absmag_r | mag | Absolute magnitude in restframe r-band from SPS SED fits | phys.magAbs |

absmag_i_stars | mag | Intrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe i-band | phys.magAbs |

absmag_i | mag | Absolute magnitude in restframe i-band from SPS SED fits | phys.magAbs |

absmag_g_stars | mag | Intrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe g-band | phys.magAbs |

absmag_g | mag | Absolute magnitude in restframe g-band from SPS SED fits | phys.magAbs |

Z_TONRY | - | Flow corrected redshift using Tonry et al. model | src.redshift |

Z | - | Heliocentric redshift | src.redshift |

SURVEY_CODE | - | Redshift source flag (5=GAMA; 1=SDSS) | meta.code;meta.dataset |

C_logM_ur | - | Correlation coefficient between logmstar and uminusi for covariant error matrix | stat.correlation |

C_logM_gi | - | Correlation coefficient between logmstar and gminusi for covariant error matrix | stat.correlation |

C_logM_eBV | - | Correlation coefficient between logmstar and extBV for covariant error matrix | stat.correlation |

CATAID | - | Unique ID of GAMA object | meta.id;meta.main |

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This DMU provides emission and absorption line measurements for all GAMA DR2 AAT spectra, as well as derived physical properties, including the star-formation rate, for all GAMA DR2 spectra and for all SDSS spectra of GAMA DR2 objects.

This is the main table of the SpecLineSFR DMU. It provides Balmer decrements, Halpha luminosities, Halpha derived star-formation rates and emission line classifications for all GAMA DR2 objects with z > -0.01 (where available).

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z_TONRY | - | Flow corrected redshift calculated from Z_HELIO_BEST using Tonry et al. model | src.redshift |

Z_HELIO_BEST | - | Heliocentric redshift of the IS_BEST spectrum | src.redshift |

Z_HELIO | - | Heliocentric redshift of the measurement spectrum | src.redshift |

WARNING_FLAG | - | Halpha or Hbeta affected by data reduction issues? | meta.code |

SURVEY_BEST | - | Survey the IS_BEST spectrum originated from | meta.code |

SURVEY | - | Survey the measurement spectrum originated from | meta.code |

SPECID_BEST | - | Unique ID of the spectrum that provides the best redshift for this object (IS_BEST spectrum) | meta.id;meta.main |

SPECID | - | Unique ID of spectrum on which line measurements were performed (measurement spectrum) | meta.id;meta.main |

SN_EMI | - | Halpha emission signal-to-noise | stat.snr |

SN_CONT | - | Continuum signal-to-noise | stat.snr |

SFR | M_sun/yr | Halpha derived star formation rate assuming a Salpeter IMF | phys.SFR;em.line.Halpha |

RA | deg | RA of GAMA object (J2000) | pos.eq.ra |

PETROMAG_R | mag | SDSS r band Petrosian magnitude (not corrected for Galactic extinction) | phot.mag;em.opt.R |

NQ_BEST | - | Normalised redshift quality of Z_HELIO_BEST | meta.code.qual;src.redshift |

NQ | - | Normalised redshift quality of Z_HELIO | meta.code.qual;src.redshift |

L_APOBSCOR | W | Halpha luminosity corrected for stellar absorption, fibre aperture effects and dust obscuration | phys.luminosity;em.line.Halpha |

L_APCOR | W | Halpha luminosity corrected for stellar absorption and fibre aperture effects | phys.luminosity;em.line.Halpha |

K_R | mag | K-correction in SDSS r band | phot.mag |

F_HBETA | 10^(-17)erg/s/cm^2 | Stellar absorption corrected Hbeta flux | spect.line.intensity;em.line.Hbeta |

F_HALPHA | 10^(-17)erg/s/cm^2 | Stellar absorption corrected Halpha flux | spect.line.intensity;em.line.Hbeta |

EMLINE_METHOD | - | AGN classification method (see notes) | meta.code |

EMLINE_CLASS | - | AGN classification based on Kewley et al. (2001) | meta.code |

DM_70_30_70 | mag | Distance modulus for 737 cosmology calculated from Z_TONRY | phot.mag.distMod |

DEC | deg | DEC of GAMA object (J2000) | pos.eq.dec |

CATAID | - | Unique ID of GAMA object | meta.id.cross;src |

BALMER_DECREMENT | - | Balmer decrement (see notes) | phot.flux;arith.ratio;spect.line |

BALMERDEC_FLAG | - | Is the Balmer decrement measured or estimated? | meta.code;phot.flux;arith.ratio |

A_R | mag | Galactic extinction in SDSS r band | phys.absorption.gal;em.opt.R |

AB_R | mag | SDSS r band absolute magnitude: PETROMAG_R - DM_70_30_70 - A_R - K_R; AB magnitude | phys.magAbs |

This table provides Balmer decrements, Halpha luminosities, Halpha derived star-formation rates and emission line classifications for all spectra in SpecLines with any measured Halpha emission and z > 0.001.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z_TONRY | - | Flow corrected redshift using Tonry et al. model | src.redshift |

Z_HELIO | - | Heliocentric redshift | src.redshift |

WARNING_FLAG | - | Halpha or Hbeta affected by data reduction issues? | meta.code |

SPECID | - | Unique spectrum ID | meta.id;meta.main |

SN_EMI | - | Halpha emission signal-to-noise | stat.snr |

SN_CONT | - | Continuum signal-to-noise | stat.snr |

SFR | M_sun/yr | Halpha derived star formation rate assuming a Salpeter IMF | phys.SFR;em.line.Halpha |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

PETROMAG_R | mag | SDSS r band Petrosian magnitude (not corrected for Galactic extinction) | phot.mag;em.opt.R |

NQ | - | Normalised redshift quality (use NQ>2 for science) | meta.code.qual;src.redshift |

L_APOBSCOR | W | Halpha luminosity corrected for stellar absorption, fibre aperture effects and dust obscuration | phys.luminosity;em.line.Halpha |

L_APCOR | W | Halpha luminosity corrected for stellar absorption and fibre aperture effects | phys.luminosity;em.line.Halpha |

K_R | mag | K-correction in SDSS r band | phot.mag |

IS_SBEST | - | Spectrum with best redshift for this object in GAMA AAT survey? | meta.code |

IS_BEST | - | Spectrum with best redshift for this object across all surveys? | meta.code |

F_HBETA | 10^(-17)erg/s/cm^2 | Stellar absorption corrected Hbeta flux | spect.line.intensity;em.line.Hbeta |

F_HALPHA | 10^(-17)erg/s/cm^2 | Stellar absorption corrected Halpha flux | spect.line.intensity;em.line.Hbeta |

EMLINE_METHOD | - | AGN classification method (see notes) | meta.code |

EMLINE_CLASS | - | AGN classification based on Kewley et al. (2001) | meta.code |

DM_70_30_70 | mag | Distance modulus for 737 cosmology | phot.mag.distMod |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

BALMER_DECREMENT | - | Balmer decrement (see notes) | phot.flux;arith.ratio;spect.line |

BALMERDEC_FLAG | - | Is the Balmer decrement measured or estimated? | meta.code;phot.flux;arith.ratio |

A_R | mag | Galactic extinction in SDSS r band | phys.absorption.gal;em.opt.R |

AB_R | mag | SDSS r band absolute magnitude: PETROMAG_R - DM_70_30_70 - A_R - K_R; AB magnitude | phys.magAbs |

This table provides Balmer decrements, Halpha luminosities, Halpha derived star-formation rates and emission line classifications for all SDSS spectra of GAMA DR2 objects with any measured Halpha emission and z > 0.001. The values in this table were derived from the MPA/JHU SDSS line measurements database.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z_TONRY | - | Flow corrected redshift using Tonry et al. model | src.redshift |

Z_HELIO_ERR | - | Redshift error | src.redshift |

Z_HELIO | - | Redshift from MPA/JHU catalogue | src.redshift |

SPECID | - | Unique spectrum ID | meta.id;meta.main |

SN_CONT | - | Continuum signal-to-noise | stat.snr |

SFR | M_sun/yr | Halpha derived star formation rate assuming a Salpeter IMF | phys.SFR;em.line.Halpha |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

PETROMAG_R | mag | SDSS r band Petrosian magnitude (not corrected for Galactic extinction) | phot.mag;em.opt.R |

MPACAT_ROWID | - | Row number of object in MPA/JHU catalogue | meta.id |

L_APOBSCOR | W | Halpha luminosity corrected for stellar absorption, fibre aperture effects and dust obscuration | phys.luminosity;em.line.Halpha |

L_APCOR | W | Halpha luminosity corrected for stellar absorption and fibre aperture effects | phys.luminosity;em.line.Halpha |

K_R | mag | K-correction in SDSS r band | phot.mag |

IS_SBEST | - | Spectrum with best redshift for this object in SDSS? | meta.code |

IS_BEST | - | Spectrum with best redshift for this object across all surveys? | meta.code |

F_HBETA | 10^(-17)erg/s/cm^2 | Stellar absorption corrected Hbeta flux | spect.line.intensity;em.line.Hbeta |

F_HALPHA | 10^(-17)erg/s/cm^2 | Stellar absorption corrected Halpha flux | spect.line.intensity;em.line.Hbeta |

EMLINE_METHOD | - | AGN classification method (see notes) | meta.code |

EMLINE_CLASS | - | AGN classification based on Kewley et al. (2001) | meta.code |

DM_70_30_70 | mag | Distance modulus for 737 cosmology | phot.mag.distMod |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

BALMER_DECREMENT | - | Balmer decrement (see notes) | phot.flux;arith.ratio;spect.line |

BALMERDEC_FLAG | - | Is the Balmer decrement measured or estimated? | meta.code;phot.flux;arith.ratio |

A_R | mag | Galactic extinction in SDSS r band | phys.absorption.gal;em.opt.R |

AB_R | mag | SDSS r band absolute magnitude: PETROMAG_R - DM_70_30_70 - A_R - K_R; AB magnitude | phys.magAbs |

This table provides emission and absorption line measurements for all GAMA DR2 AAT spectra with a redshift measurement.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z_HELIO | - | Spectroscopic redshift | src.redshift |

SPECID | - | Unique spectrum ID | meta.id;meta.main |

SIIRSIGERR | A | [SII] 6731A sigma error | stat.error;spect.line.width |

SIIRSIG | A | [SII] 6731A sigma | spect.line.width |

SIIREW | A | [SII] 6731A equivalent width (see notes) | spect.line.eqWidth |

SIIRERR | 10^(-17)erg/s/cm^2 | [SII] 6731A line flux error | stat.error;spect.line.intensity |

SIIR | 10^(-17)erg/s/cm^2 | [SII] 6731A line flux (Gaussian fit, see notes) | spect.line.intensity |

SIIBSIGERR | A | [SII] 6716A sigma error | stat.error;spect.line.width |

SIIBSIG | A | [SII] 6716A sigma | spect.line.width |

SIIBEW | A | [SII] 6716A equivalent width (see notes) | spect.line.eqWidth |

SIIBERR | 10^(-17)erg/s/cm^2 | [SII] 6716A line flux error | stat.error;spect.line.intensity |

SIIB | 10^(-17)erg/s/cm^2 | [SII] 6716A line flux (Gaussian fit, see notes) | spect.line.intensity |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

OIIRSIGERR | A | [OII] 3727A sigma error | stat.error;spect.line.width |

OIIRSIG | A | [OII] 3727A sigma | spect.line.width |

OIIREW | A | [OII] 3727A equivalent width (see notes) | spect.line.eqWidth |

OIIRERR | 10^(-17)erg/s/cm^2 | [OII] 3727A line flux error | stat.error;spect.line.intensity |

OIIR | 10^(-17)erg/s/cm^2 | [OII] 3727A line flux (double Gaussian fit to red peak, see notes) | spect.line.intensity |

OIIIRSIGERR | A | [OIII] 5007A sigma error | stat.error;spect.line.width;em.line.OIII |

OIIIRSIG | A | [OIII] 5007A sigma | spect.line.width;em.line.OIII |

OIIIREW | A | [OIII] 5007A equivalent width (see notes) | spect.line.eqWidth;em.line.OIII |

OIIIRERR | 10^(-17)erg/s/cm^2 | [OIII] 5007A line flux error | stat.error;spect.line.intensity;em.li... |

OIIIR | 10^(-17)erg/s/cm^2 | [OIII] 5007A line flux (Gaussian fit, see notes) | spect.line.intensity;em.line.OIII |

OIIIBSIGERR | A | [OIII] 4959A sigma error | stat.error;spect.line.width |

OIIIBSIG | A | [OIII] 4959A sigma | spect.line.width |

OIIIBEW | A | [OIII] 4959A equivalent width (see notes) | spect.line.eqWidth |

OIIIBERR | 10^(-17)erg/s/cm^2 | [OIII] 4959A line flux error | stat.error;spect.line.intensity |

OIIIB | 10^(-17)erg/s/cm^2 | [OIII] 4959A line flux (Gaussian fit, see notes) | spect.line.intensity |

OIIERR | 10^(-17)erg/s/cm^2 | [OII] 3727A line flux error (Gaussian fit) | stat.error;spect.line.intensity |

OIIBSIGERR | A | [OII] 3727A sigma error | stat.error;spect.line.width |

OIIBSIG | A | [OII] 3727A sigma | spect.line.width |

OIIBEW | A | [OII] 3727A equivalent width (see notes) | spect.line.eqWidth |

OIIBERR | 10^(-17)erg/s/cm^2 | [OII] 3727A line flux error | stat.error;spect.line.intensity |

OIIB | 10^(-17)erg/s/cm^2 | [OII] 3727A line flux (double Gaussian fit to blue peak, see notes) | spect.line.intensity |

OII | 10^(-17)erg/s/cm^2 | [OII] 3727A line flux (Gaussian fit, see notes) | spect.line.intensity |

NQ | - | Quality flag (4 is reliable, 3 tentative) | meta.code.qual;src.redshift |

NIIRSIGERR | A | [NII] 6584A sigma error | stat.error;spect.line.width |

NIIRSIG | A | [NII] 6584A sigma | spect.line.width |

NIIREW | A | [NII] 6584A equivalent width (see notes) | spect.line.eqWidth |

NIIRERR | 10^(-17)erg/s/cm^2 | [NII] 6584A line flux error | stat.error;spect.line.intensity |

NIIR | 10^(-17)erg/s/cm^2 | [NII] 6584A line flux (Gaussian fit, see notes) | spect.line.intensity |

NIIBSIGERR | A | [NII] 6548A sigma error | stat.error;spect.line.width |

NIIBSIG | A | [NII] 6548A sigma | spect.line.width |

NIIBEW | A | [NII] 6548A equivalent width (see notes) | spect.line.eqWidth |

NIIBERR | 10^(-17)erg/s/cm^2 | [NII] 6548A line flux error | stat.error;spect.line.intensity |

NIIB | 10^(-17)erg/s/cm^2 | [NII] 6548A line flux (Gaussian fit, see notes) | spect.line.intensity |

IS_SBEST | - | Spectrum with best redshift for this object in GAMA AAT survey? | meta.code |

IS_BEST | - | Spectrum with best redshift for this object across all surveys? | meta.code |

ISIIRERR | 10^(-17)erg/s/cm^2 | [SII] 6731A integrated line flux error | stat.error;phot.flux;spect.line |

ISIIR | 10^(-17)erg/s/cm^2 | [SII] 6731A integrated line flux (see notes) | phot.flux;spect.line |

ISIIBERR | 10^(-17)erg/s/cm^2 | [SII] 6716A integrated line flux error | stat.error;phot.flux;spect.line |

ISIIB | 10^(-17)erg/s/cm^2 | [SII] 6716A integrated line flux (see notes) | phot.flux;spect.line |

IOIIIRERR | 10^(-17)erg/s/cm^2 | [OIII] 5007A integrated line flux error | stat.error;phot.flux;em.line.OIII |

IOIIIR | 10^(-17)erg/s/cm^2 | [OIII] 5007A integrated line flux (see notes) | phot.flux;em.line.OIII |

IOIIIBERR | 10^(-17)erg/s/cm^2 | [OIII] 4959A integrated line flux error | stat.error;phot.flux;spect.line |

IOIIIB | 10^(-17)erg/s/cm^2 | [OIII] 4959A integrated line flux (see notes) | phot.flux;spect.line |

IOIIERR | 10^(-17)erg/s/cm^2 | [OII] 3727A integrated line flux error | stat.error;phot.flux;spect.line |

IOII | 10^(-17)erg/s/cm^2 | [OII] 3727A integrated line flux (see notes) | phot.flux;spect.line |

IOI6364ERR | 10^(-17)erg/s/cm^2 | [OI] 6364A integrated line flux error | stat.error;phot.flux;spect.line |

IOI6364 | 10^(-17)erg/s/cm^2 | [OI] 6364A integrated line flux (see notes) | phot.flux;spect.line |

IOI6300ERR | 10^(-17)erg/s/cm^2 | [OI] 6300A integrated line flux error | stat.error;phot.flux;spect.line |

IOI6300 | 10^(-17)erg/s/cm^2 | [OI] 6300A integrated line flux (see notes) | phot.flux;spect.line |

INIIRERR | 10^(-17)erg/s/cm^2 | [NII] 6584A integrated line flux error | stat.error;phot.flux;spect.line |

INIIR | 10^(-17)erg/s/cm^2 | [NII] 6584A integrated line flux (see notes) | phot.flux;spect.line |

INIIBERR | 10^(-17)erg/s/cm^2 | [NII] 6548A integrated line flux error | stat.error;phot.flux;spect.line |

INIIB | 10^(-17)erg/s/cm^2 | [NII] 6548A integrated line flux (see notes) | phot.flux;spect.line |

INEVRERR | 10^(-17)erg/s/cm^2 | [NeV] 3425A integrated line flux error | stat.error;phot.flux;spect.line |

INEVR | 10^(-17)erg/s/cm^2 | [NeV] 3425A integrated line flux (see notes) | phot.flux;spect.line |

INEVBERR | 10^(-17)erg/s/cm^2 | [NeV] 3345A integrated line flux error | stat.error;phot.flux;spect.line |

INEVB | 10^(-17)erg/s/cm^2 | [NeV] 3345A integrated line flux (see notes) | phot.flux;spect.line |

INEIIIERR | 10^(-17)erg/s/cm^2 | [NeIII] 3869A integrated line flux error | stat.error;phot.flux;spect.line |

INEIII | 10^(-17)erg/s/cm^2 | [NeIII] 3869A integrated line flux (see notes) | phot.flux;spect.line |

INADERR | 10^(-17)erg/s/cm^2 | NaID 5892A integrated line flux error | stat.error;phot.flux;spect.line |

INAD | 10^(-17)erg/s/cm^2 | NaID 5892A integrated line flux (see notes) | phot.flux;spect.line |

IMGERR | 10^(-17)erg/s/cm^2 | Mg 5174A integrated line flux error | stat.error;phot.flux;spect.line |

IMG | 10^(-17)erg/s/cm^2 | Mg 5174A integrated line flux (see notes) | phot.flux;spect.line |

IHDERR | 10^(-17)erg/s/cm^2 | Hdelta integrated line flux error | stat.error;phot.flux;spect.line |

IHD | 10^(-17)erg/s/cm^2 | Hdelta integrated line flux (see notes) | phot.flux;spect.line |

IHBERR | 10^(-17)erg/s/cm^2 | Hbeta integrated line flux error | stat.error;phot.flux;em.line.Hbeta |

IHB | 10^(-17)erg/s/cm^2 | Hbeta integrated line flux (see notes) | phot.flux;em.line.Hbeta |

IHAERR | 10^(-17)erg/s/cm^2 | Halpha integrated line flux error | stat.error;phot.flux;em.line.Halpha |

IHA | 10^(-17)erg/s/cm^2 | Halpha integrated line flux (see notes) | phot.flux;em.line.Halpha |

HBSIGERR | A | Hbeta sigma error | stat.error;spect.line.width;em.line.H... |

HBSIG | A | Hbeta sigma | spect.line.width;em.line.Hbeta |

HBEW | A | Hbeta equivalent width (see notes) | spect.line.eqWidth;em.line.Hbeta |

HBERR | 10^(-17)erg/s/cm^2 | Hbeta line flux error (Gaussian fit) | stat.error;spect.line.intensity;em.li... |

HB | 10^(-17)erg/s/cm^2 | Hbeta line flux (Gaussian fit, see notes) | spect.line.intensity;em.line.Hbeta |

HASIGERR | A | Halpha sigma error | stat.error;spect.line.width;em.line.H... |

HASIG | A | Halpha sigma | spect.line.width;em.line.Halpha |

HAEW | A | Halpha equivalent width (see notes) | spect.line.eqWidth;em.line.Halpha |

HAERR | 10^(-17)erg/s/cm^2 | Halpha line flux error (Gaussian fit) | stat.error;spect.line.intensity;em.li... |

HA | 10^(-17)erg/s/cm^2 | Halpha line flux (Gaussian fit, see notes) | spect.line.intensity;em.line.Halpha |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

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This DMU provides the final spectra and redshift catalogues, including GAMA AAT and external data.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

ZDSTART | deg | Zenith distance at start of first exposure | pos.az.zd;time.start |

ZDEND | deg | Zenith distance at end of last exposure | pos.az.zd;time.rnd |

UTSTART | hms | UT of start of first exposure | time.start;obs.exposure |

UTMJD | - | Mean MJD of start of exposures | time.epoch;obs.exposure |

UTEND | hms | UT of end of last exposure | time.end;obs.exposure |

USER | - | Original redshifter of this field | meta.id |

T_EXP | s | Total exposure time | time.duration;obs.exposure |

TDFDRVER | - | Version of 2dfdr data reduction software | meta.version;meta.software |

RA | deg | RA of field centre (J2000) | pos.eq.ra;obs.field |

PLATE | - | 2dF plate number | meta.id;instr |

N_STAR | - | Number of calibration stars observed | meta.number;src.calib |

N_SPEC | - | Number of spectra observed | meta.number;spect |

N_NIGHTS | - | Number of nights over which exposures were spread | meta.number |

N_GOOD | - | Number of spectra with a good quality redshift, i.e. nQ >= 3 | meta.number;spect |

N_GAL_GOOD | - | Number of galaxy target spectra with a good quality redshift, i.e. nQ >= 3 | meta.number;src |

N_GAL | - | Number of galaxy targets observed | meta.number;src |

N_EXP | - | Number of exposures | meta.number;obs.exposure |

MEAN_SN | - | Mean S/N of spectra | stat.snr;spect |

HEL_VC | km/s | Heliocentric velocity correction | phys.velocity;pos.heliocentric |

HASTART | deg | Hour angle at start of first exposure | pos.eq.ha;time.start |

HAEND | deg | Hour angle at end of last exposure | pos.eq.ha;time.end |

GAL_COMPL | - | Redshift success rate among galaxy targets | arith.ratio;meta.number;src |

FIELDID | - | ID of GAMA AAT field | meta.id;obs.field |

DEC | deg | DEC of field centre (J2000) | pos.eq.dec;obs.field |

DATE_Z | iso-8601 | Date of original redshifting run | time.processing |

DATE_OBS | iso-8601 | UT date of observation | time.epoch;obs.exposure |

CRCORVER | - | Runz version used for original redshifting run | meta.version;meta.software |

CONFIG_FILE | - | Name of configuration file | meta.id;meta.file;instr.setup |

COMPL | - | Redshift success rate | arith.ratio;meta.number;spect |

This table contains the complete output of the redshifting code for all spectra released in DR2. Note that many spectra were redshifted more than once and this catalogue contains all duplications.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z_FIN_ERR | - | Error of final selected redshift | stat.error;src.redshift |

Z_FIN | - | Final selected redshift | src.redshift |

ZX_ERR | - | Cross-correlation redshift error | - |

ZX | - | Cross-correlation redshift | - |

ZEM_ERR | - | Emission line redshift error | - |

ZEM | - | Emission line redshift | - |

Y_POSN | - | Fibre y position on plate | - |

X_POSN | - | Fibre x position on plate | - |

XCOR | - | Cross-correlation peak height | - |

VSP | mag | Approximate V-band fibre mag with zeropoint 32 | - |

USER | - | Redshifter | meta.id |

TEMP | - | Cross-correlation template | - |

S_N | - | S/N of spectrum | stat.snr |

SPMAG | mag | Unused | - |

SPECID | - | ID of GAMA AAT spectrum | meta.id;spect |

RUNZRESID | - | ID of runz output | meta.id;meta.main |

RSP | mag | Approximate R-band fibre mag with zeropoint 32.3 | - |

RMAG | mag | Extinction corrected SDSS r-band Petrosian magnitude | phot.mag;em.opt.R |

RAS | s | RA seconds | - |

RAM | m | RA minutes | - |

RAH | h | RA hours of spectrum (J2000) | - |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

QX | - | Cross-correlation redshift quality | - |

QOP | - | User assigned quality of final selected redshift | meta.code.qual;src.redshift |

QEM | - | Emission line redshift quality | - |

QA | - | Automatic quality of final selected redshift | - |

PLATE | - | Plate number | meta.id;instr |

OBJECT | - | Object name | - |

NEG | - | Total number of detected potential emission lines | - |

NEB | - | Number of matching emission lines at best emission line redshift | - |

IC_FLAG | - | Catalogue source(s) of matched GAMA object | meta.code.member |

GAMA_NAME | - | Name of matched GAMA object | meta.id.cross;src |

FLD | - | Unused | - |

FIELDID | - | ID of GAMA AAT field | meta.id;obs.field |

FIBRE | - | Fibre number | meta.id;instr |

F | - | Flag indicating whether Z_FIN is different from automatic redshifts: 0 = equal to best auto redshift; 1 = not equal to best auto redshift; 2 = not equal to either auto redshifts | meta.code |

DIST | arcsec | Distance between spectrum and matched GAMA object | pos.angDistance |

DECS | s | DEC seconds | - |

DECM | m | DEC minutes | - |

DECD | deg | DEC degree of spectrum (J2000) | - |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

DATE_Z | iso-8601 | Date of runz run | time.processing |

DATE_OBS | - | UT date of observation | time.epoch;obs.exposure |

COMMENT | - | User comment | meta.note |

CCD | - | CCD number | meta.id;instr |

CATAID | - | ID of matched GAMA object | meta.id.cross;src |

This is a table of all GAMA AAT spectra included in DR2. Many targets were observed more than once by GAMA, and these duplications are retained here.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z | - | Heliocentric redshift | src.redshift |

Y_POSN | - | Fibre y position on plate | - |

X_POSN | - | Fibre x position on plate | - |

WMIN | A | Minimum wavelength of spectrum | em.wl;stat.min |

WMAX | A | Maximum wavelength of spectrum | em.wl;stat.max |

URL_IMG | - | URL of the spectrum`s image | meta.ref.url;meta.file |

URL | - | URL of the spectrum | meta.ref.url;meta.file;meta.fits |

S_N | - | S/N of spectrum | stat.snr |

SPECID | - | ID of GAMA AAT spectrum | meta.id;meta.main |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

PROB | - | Probability that redshift is correct | stat.probability;src.redshift |

PLATE | - | Plate number | meta.id;instr |

NQ | - | Normalised redshift quality (use nQ > 2 for science) | meta.code.qual;src.redshift |

IS_SBEST | - | Is this the best GAMA AAT spectrum of this object? | meta.code |

IC_FLAG | - | Catalogue source(s) of matched GAMA object | meta.code.member |

GAMA_NAME | - | Name of matched GAMA object | meta.id.cross;src |

FILENAME | - | Full path and filename of the spectrum | meta.id;meta.file;meta.fits |

FIELDID | - | ID of GAMA AAT field | meta.id;obs.field |

FIBRE | - | Fibre number | meta.id;instr |

DIST | arcsec | Distance between spectrum and matched GAMA object | pos.angDistance |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

DATE_OBS | iso-8601 | UT date of observation | time.epoch;obs.exposure |

CATAID | - | ID of matched GAMA object | meta.id.cross;src |

Many GAMA AAT spectra were redshifted more than once. For each spectrum included in DR2 this table contains one line summarising all of the redshifting results for this spectrum, as well as listing the results of the analysis to determine the best redshift based on the reliabilities of the redshifters.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z4_Z | - | Possible redshift | - |

Z4_PROB | - | Probability that ZX_Z is correct | - |

Z4_N_Q4 | - | Number of supporting Q=4 opinions | - |

Z4_N_Q3 | - | Number of supporting Q=3 opinions | - |

Z4_N_Q2 | - | Number of supporting Q=2 opinions | - |

Z4_NQ | - | Normalised Q of ZX_Z | - |

Z4_N | - | Number of opinions supporting ZX_Z | - |

Z3_Z | - | Possible redshift | - |

Z3_PROB | - | Probability that ZX_Z is correct | - |

Z3_N_Q4 | - | Number of supporting Q=4 opinions | - |

Z3_N_Q3 | - | Number of supporting Q=3 opinions | - |

Z3_N_Q2 | - | Number of supporting Q=2 opinions | - |

Z3_NQ | - | Normalised Q of ZX_Z | - |

Z3_N | - | Number of opinions supporting ZX_Z | - |

Z2_Z | - | Possible redshift | - |

Z2_PROB | - | Probability that ZX_Z is correct | - |

Z2_N_Q4 | - | Number of supporting Q=4 opinions | - |

Z2_N_Q3 | - | Number of supporting Q=3 opinions | - |

Z2_N_Q2 | - | Number of supporting Q=2 opinions | - |

Z2_NQ | - | Normalised Q of ZX_Z | - |

Z2_N | - | Number of opinions supporting ZX_Z | - |

Z1_Z | - | Possible redshift | - |

Z1_PROB | - | Probability that ZX_Z is correct | - |

Z1_N_Q4 | - | Number of supporting Q=4 opinions | - |

Z1_N_Q3 | - | Number of supporting Q=3 opinions | - |

Z1_N_Q2 | - | Number of supporting Q=2 opinions | - |

Z1_NQ | - | Normalised Q of ZX_Z | - |

Z1_N | - | Number of opinions supporting ZX_Z | - |

SPECID | - | ID of GAMA AAT spectrum | meta.id;meta.main |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

Q1_PROB | - | Probability that the possibility Q=1 is correct | stat.probability |

Q1_N_Q1 | - | Number of supporting Q=1 opinions | meta.number |

Q1_N_Q0 | - | Number of supporting Q=0 opinions | meta.number |

OP5_ZIDX | - | Index of possibility in above list that is supported by this redshift | - |

OP5_Z | - | Redshift | - |

OP5_RUNZRESID | - | ID of additional runz result in AATRunzResults | - |

OP5_RS | - | Redshifter | - |

OP5_Q | - | Q | - |

OP4_ZIDX | - | Index of possibility in above list that is supported by this redshift | - |

OP4_Z | - | Redshift | - |

OP4_RUNZRESID | - | ID of additional runz result in AATRunzResults | - |

OP4_RS | - | Redshifter | - |

OP4_Q | - | Q | - |

OP3_ZIDX | - | Index of possibility in above list that is supported by this redshift | - |

OP3_Z | - | Redshift | - |

OP3_RUNZRESID | - | ID of additional runz result in AATRunzResults | - |

OP3_RS | - | Redshifter | - |

OP3_Q | - | Q | - |

OP2_ZIDX | - | Index of possibility in above list that is supported by this redshift | - |

OP2_Z | - | Redshift | - |

OP2_RUNZRESID | - | ID of additional runz result in AATRunzResults | - |

OP2_RS | - | Redshifter | - |

OP2_Q | - | Q | - |

OP1_ZIDX | - | Index of possibility in above list that is supported by this redshift | - |

OP1_Z | - | Original redshift | - |

OP1_RUNZRESID | - | ID of original runz result in AATRunzResults | - |

OP1_RS | - | Original redshifter | - |

OP1_Q | - | Original Q | - |

N_Z | - | Number of different redshifts | meta.number |

N_OPQG | - | Number of opinions with Q >= 2 | meta.number |

N_OPQB | - | Number of opinions with Q < 2 | meta.number |

N_OP | - | Number of opinions for this spectrum | meta.number |

IC_FLAG | - | Catalogue source(s) of matched GAMA object | meta.code.member |

GAMA_NAME | - | Name of matched GAMA object | meta.id.cross;src |

FIELDID | - | ID of GAMA AAT field | meta.id;obs.field |

DIST | arcsec | Distance between spectrum and matched GAMA object | pos.angDistance |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

COMP_PROB | - | Probability that all offered possibilities are wrong | stat.probability |

CATAID | - | ID of matched GAMA object | meta.id.cross;src |

BEST_Z_N_Q4 | - | Number of supporting Q=4 opinions | meta.number |

BEST_Z_N_Q3 | - | Number of supporting Q=3 opinions | meta.number |

BEST_Z_N_Q2 | - | Number of supporting Q=2 opinions | meta.number |

BEST_Z_N_Q1 | - | Number of supporting Q=1 opinions | meta.number |

BEST_Z_N_Q0 | - | Number of supporting Q=0 opinions | meta.number |

BEST_Z_NQ | - | Normalised Q of the most probable possibility | meta.code.qual;src.redshift |

BEST_Z_N | - | Number of opinions supporting the most probable possibility | meta.number |

BEST_Z | - | Redshift of the most probable possibility | src.redshift |

BEST_PROB | - | Probability that the most probable possibility is correct | stat.probability;src.redshift |

BEST_IDX | - | Index of best possibility in the above list | - |

This table lists a small number of spectra of fibre-bright targets collected by the GAMA team at the Liverpool Telescope (LT).

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z | - | Heliocentric redshift | src.redshift |

WMIN | A | Minimum wavelength of spectrum | em.wl;stat.min |

WMAX | A | Maximum wavelength of spectrum | em.wl;stat.max |

URL_IMG | - | URL of the spectrum`s image | meta.ref.url;meta.file |

URL | - | URL of the spectrum | meta.ref.url;meta.file;meta.fits |

SPECID | - | ID of GAMA LT spectrum | meta.id;meta.main |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

PROB | - | Probability that redshift is correct | stat.probability;src.redshift |

NQ | - | Normalised redshift quality (use nQ > 2 for science) | meta.code.qual;src.redshift |

IS_SBEST | - | Is this the best GAMA LT spectrum of this object? | meta.code |

IC_FLAG | - | Catalogue source(s) of matched GAMA object | meta.code.member |

GAMA_NAME | - | Name of matched GAMA object | meta.id.cross;src |

FILENAME | - | Full path and filename of the spectrum | meta.id;meta.file;meta.fits |

DIST | arcsec | Distance between spectrum and matched GAMA object | pos.angDistance |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

CATAID | - | ID of matched GAMA object | meta.id.cross;src |

This table lists all spectra that are available for GAMA objects included in DR2, including GAMA spectra and those from previous spectroscopic surveys (such as the SDSS). Duplicate observations of the same object are retained in this table (but a flag is provided to mark the spectrum that provided the best available redshift of a given object). Every spectrum listed in this table is available in the GAMA DR2 database.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z | - | Heliocentric redshift | src.redshift |

WMIN | A | Minimum wavelength of spectrum | em.wl;stat.min |

WMAX | A | Maximum wavelength of spectrum | em.wl;stat.max |

URL_IMG | - | URL of the spectrum`s image | meta.ref.url;meta.file |

URL | - | URL of the spectrum | meta.ref.url;meta.file;meta.fits |

SURVEY_CODE | - | Numerical code for originating survey | meta.code;meta.dataset |

SURVEY | - | Survey this spectrum originated from | meta.dataset |

SPECID | - | Unique ID of spectrum | meta.id;meta.main |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

PROB | - | Probability that redshift is correct | stat.probability;src.redshift |

NQ | - | Normalised redshift quality (use nQ > 2 for science) | meta.code.qual;src.redshift |

IS_SBEST | - | Is this the best spectrum of this GAMA object within the originating survey? | meta.code |

IS_BEST | - | Is this the best spectrum of this GAMA object? | meta.code |

IC_FLAG | - | Catalogue source(s) of matched GAMA object | meta.code.member |

GAMA_NAME | - | Name of matched GAMA object | meta.id.cross;src |

FILENAME | - | Full path and filename of the spectrum | meta.id;meta.file;meta.fits |

DIST | arcsec | Distance between spectrum and matched GAMA object | pos.angDistance |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

CATAID | - | ID of matched GAMA object | meta.id.cross;src |

This table lists each observed target included in DR2 and the spectrum that provides its best redshift (from GAMA or otherwise).

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

Z | - | Heliocentric redshift | src.redshift |

WMIN | A | Minimum wavelength of spectrum | em.wl;stat.min |

WMAX | A | Maximum wavelength of spectrum | em.wl;stat.max |

URL_IMG | - | URL of the spectrum`s image | meta.ref.url;meta.file |

URL | - | URL of the spectrum | meta.ref.url;meta.file;meta.fits |

SURVEY_CODE | - | Numerical code for originating survey | meta.code;meta.dataset |

SURVEY | - | Survey this spectrum originated from | meta.dataset |

SPECID | - | ID of best matched spectrum | meta.id.cross;spect |

RA | deg | RA of spectrum (J2000) | pos.eq.ra |

PROB | - | Probability that redshift is correct | stat.probability;src.redshift |

N_SPEC | - | Number of spectra available for this object | meta.number;spect |

N_GAMA_SPEC | - | Number of GAMA spectra available for this object | meta.number;spect |

NQ | - | Normalised redshift quality (use nQ > 2 for science) | meta.code.qual;src.redshift |

IC_FLAG | - | Catalogue source(s) of GAMA object | meta.code.member |

GAMA_NAME | - | Name of GAMA object | meta.id |

FILENAME | - | Full path and filename of the spectrum | meta.id;meta.file;meta.fits |

DIST | arcsec | Distance between GAMA object and best matched spectrum | pos.angDistance |

DEC | deg | DEC of spectrum (J2000) | pos.eq.dec |

CATAID | - | Unique ID of GAMA object | meta.id;meta.main |

read more
This DMU provides a single-component Sersic fit in each of the ugrizYJHK bands for every GAMA DR2 galaxy.

This catalogue contains the most useful subset of the output of the SersicPhotometry DMU, using SIGMA v0.9-0 (Structural Investigation of Galaxies via Model Analysis) to generate a single-Sersic fit to every GAMA DR2 object. This table is an exact subset of the table SersicCatAll.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

URL_R | - | URL of r-band png file | meta.ref.url;meta.file |

URL_K | - | URL of K-band png file | meta.ref.url;meta.file |

URL | - | URL of the object`s data dir | meta.ref.url;meta.file |

SIGMA_INDEX | - | SIGMA Object ID (see notes) | meta.id |

RA | deg | Right Ascension (J2000) | pos.eq.ra |

PSF_FWHM_Z | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.opt |

PSF_FWHM_Y | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.IR.NIR |

PSF_FWHM_U | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.opt.U |

PSF_FWHM_R | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.opt.R |

PSF_FWHM_K | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.IR.K |

PSF_FWHM_J | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.IR.J |

PSF_FWHM_I | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.opt.I |

PSF_FWHM_H | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.IR.H |

PSF_FWHM_G | arcsec | PSFEx PSF FWHM | instr.det.psf;meta.modelled;em.opt |

OBJNAME | - | SIGMA Object name (see notes) | meta.id |

GAL_YCEN_Z | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.opt |

GAL_YCEN_Y | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.IR.NIR |

GAL_YCEN_U | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.opt.U |

GAL_YCEN_R | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.opt.R |

GAL_YCEN_K | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.IR.K |

GAL_YCEN_J | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.IR.J |

GAL_YCEN_I | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.opt.I |

GAL_YCEN_H | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.IR.H |

GAL_YCEN_G | pixel | pixel pos. of model in cutout (y) | pos.cartesian.y;meta.modelled;em.opt |

GAL_XCEN_Z | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.opt |

GAL_XCEN_Y | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.IR.NIR |

GAL_XCEN_U | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.opt.U |

GAL_XCEN_R | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.opt.R |

GAL_XCEN_K | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.IR.K |

GAL_XCEN_J | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.IR.J |

GAL_XCEN_I | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.opt.I |

GAL_XCEN_H | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.IR.H |

GAL_XCEN_G | pixel | pixel pos. of model in cutout (x) | pos.cartesian.x;meta.modelled;em.opt |

GAL_RE_Z | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt |

GAL_RE_Y | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.NIR |

GAL_RE_U | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt.U |

GAL_RE_R | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt.R |

GAL_RE_K | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.K |

GAL_RE_J | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.J |

GAL_RE_I | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt.I |

GAL_RE_H | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.H |

GAL_RE_G | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt |

GAL_RE_C_Z | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt |

GAL_RE_C_Y | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.NIR |

GAL_RE_C_U | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt.U |

GAL_RE_C_R | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt.R |

GAL_RE_C_K | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.K |

GAL_RE_C_J | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.J |

GAL_RE_C_I | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt.I |

GAL_RE_C_H | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.H |

GAL_RE_C_G | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt |

GAL_RA_Z | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt |

GAL_RA_Y | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.NIR |

GAL_RA_U | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt.U |

GAL_RA_R | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt.R |

GAL_RA_K | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.K |

GAL_RA_J | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.J |

GAL_RA_I | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt.I |

GAL_RA_H | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.H |

GAL_RA_G | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt |

GAL_R90_Z | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt |

GAL_R90_Y | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.NIR |

GAL_R90_U | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt.U |

GAL_R90_R | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt.R |

GAL_R90_K | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.K |

GAL_R90_J | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.J |

GAL_R90_I | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt.I |

GAL_R90_H | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.H |

GAL_R90_G | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt |

GAL_PA_Z | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt |

GAL_PA_Y | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.NIR |

GAL_PA_U | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt.U |

GAL_PA_R | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt.R |

GAL_PA_K | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.K |

GAL_PA_J | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.J |

GAL_PA_I | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt.I |

GAL_PA_H | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.H |

GAL_PA_G | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt |

GAL_MU_E_Z | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_E_Y | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.NIR |

GAL_MU_E_U | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt.U |

GAL_MU_E_R | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt.R |

GAL_MU_E_K | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.K |

GAL_MU_E_J | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.J |

GAL_MU_E_I | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt.I |

GAL_MU_E_H | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.H |

GAL_MU_E_G | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_E_AVG_Z | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_E_AVG_Y | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.NIR |

GAL_MU_E_AVG_U | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt.U |

GAL_MU_E_AVG_R | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt.R |

GAL_MU_E_AVG_K | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.K |

GAL_MU_E_AVG_J | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.J |

GAL_MU_E_AVG_I | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt.I |

GAL_MU_E_AVG_H | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.H |

GAL_MU_E_AVG_G | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_0_Z | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_0_Y | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.NIR |

GAL_MU_0_U | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt.U |

GAL_MU_0_R | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt.R |

GAL_MU_0_K | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.K |

GAL_MU_0_J | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.J |

GAL_MU_0_I | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt.I |

GAL_MU_0_H | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.H |

GAL_MU_0_G | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt |

GAL_MAG_Z | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt |

GAL_MAG_Y | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.NIR |

GAL_MAG_U | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt.U |

GAL_MAG_R | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt.R |

GAL_MAG_K | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.K |

GAL_MAG_J | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.J |

GAL_MAG_I | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt.I |

GAL_MAG_H | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.H |

GAL_MAG_G | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt |

GAL_MAG_10RE_Z | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt |

GAL_MAG_10RE_Y | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.NIR |

GAL_MAG_10RE_U | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt.U |

GAL_MAG_10RE_R | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt.R |

GAL_MAG_10RE_K | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.K |

GAL_MAG_10RE_J | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.J |

GAL_MAG_10RE_I | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt.I |

GAL_MAG_10RE_H | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.H |

GAL_MAG_10RE_G | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt |

GAL_INDEX_Z | - | Sersic index | stat.fit.param;meta.modelled;em.opt |

GAL_INDEX_Y | - | Sersic index | stat.fit.param;meta.modelled;em.IR.NIR |

GAL_INDEX_U | - | Sersic index | stat.fit.param;meta.modelled;em.opt.U |

GAL_INDEX_R | - | Sersic index | stat.fit.param;meta.modelled;em.opt.R |

GAL_INDEX_K | - | Sersic index | stat.fit.param;meta.modelled;em.IR.K |

GAL_INDEX_J | - | Sersic index | stat.fit.param;meta.modelled;em.IR.J |

GAL_INDEX_I | - | Sersic index | stat.fit.param;meta.modelled;em.opt.I |

GAL_INDEX_H | - | Sersic index | stat.fit.param;meta.modelled;em.IR.H |

GAL_INDEX_G | - | Sersic index | stat.fit.param;meta.modelled;em.opt |

GAL_ELLIP_Z | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.opt |

GAL_ELLIP_Y | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.IR.NIR |

GAL_ELLIP_U | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.opt.U |

GAL_ELLIP_R | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.opt.R |

GAL_ELLIP_K | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.IR.K |

GAL_ELLIP_J | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.IR.J |

GAL_ELLIP_I | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.opt.I |

GAL_ELLIP_H | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.IR.H |

GAL_ELLIP_G | - | ellipticity (1-(b/a)) | src.ellipticity;meta.modelled;em.opt |

GAL_DEC_Z | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.opt |

GAL_DEC_Y | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.IR.NIR |

GAL_DEC_U | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.opt.U |

GAL_DEC_R | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.opt.R |

GAL_DEC_K | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.IR.K |

GAL_DEC_J | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.IR.J |

GAL_DEC_I | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.opt.I |

GAL_DEC_H | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.IR.H |

GAL_DEC_G | deg | Declination as determined by GALFIT | pos.eq.dec;meta.modelled;em.opt |

GAL_CHI2_Z | - | reduced Chi^2 of output model | stat.fit.goodness;em.opt |

GAL_CHI2_Y | - | reduced Chi^2 of output model | stat.fit.goodness;em.IR.NIR |

GAL_CHI2_U | - | reduced Chi^2 of output model | stat.fit.goodness;em.opt.U |

GAL_CHI2_R | - | reduced Chi^2 of output model | stat.fit.goodness;em.opt.R |

GAL_CHI2_K | - | reduced Chi^2 of output model | stat.fit.goodness;em.IR.K |

GAL_CHI2_J | - | reduced Chi^2 of output model | stat.fit.goodness;em.IR.J |

GAL_CHI2_I | - | reduced Chi^2 of output model | stat.fit.goodness;em.opt.I |

GAL_CHI2_H | - | reduced Chi^2 of output model | stat.fit.goodness;em.IR.H |

GAL_CHI2_G | - | reduced Chi^2 of output model | stat.fit.goodness;em.opt |

FILENAME | - | Full path to object`s data directory | meta.id;meta.file |

DEC | deg | Declination (J2000) | pos.eq.dec |

CATAID | - | GAMA Object ID | meta.id |

This catalogue contains the complete output of the SersicPhotometry DMU, using SIGMA v0.9-0 (Structural Investigation of Galaxies via Model Analysis) to generate a single-Sersic fit to every GAMA DR2 object.

Name | Unit | Description | UCD (hover for description) |
---|---|---|---|

Name | Unit | Description | UCD |

GAL_RUN_H | - | number of GALFIT runs required | meta.number;em.IR.H |

GAL_RUN_G | - | number of GALFIT runs required | meta.number;em.opt |

GAL_RE_Z | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt |

GAL_RE_Y | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.NIR |

GAL_RE_U | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt.U |

GAL_RE_R | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt.R |

GAL_RE_K | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.K |

GAL_RE_J | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.J |

GAL_RE_I | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt.I |

GAL_RE_H | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.IR.H |

GAL_RE_G | arcsec | effective radius (hl rad) (semi-major) | phys.angSize;meta.modelled;em.opt |

GAL_RE_ERR_Z | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_Y | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_U | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_R | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_K | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_J | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_I | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_H | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_ERR_G | arcsec | GALFIT error on re | phys.angSize;stat.error;meta.modelled... |

GAL_RE_C_Z | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt |

GAL_RE_C_Y | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.NIR |

GAL_RE_C_U | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt.U |

GAL_RE_C_R | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt.R |

GAL_RE_C_K | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.K |

GAL_RE_C_J | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.J |

GAL_RE_C_I | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt.I |

GAL_RE_C_H | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.IR.H |

GAL_RE_C_G | arcsec | circularised effective radius | phys.angSize;meta.modelled;em.opt |

GAL_RESULT_Z | - | GALFIT run result (see notes) | em.opt |

GAL_RESULT_Y | - | GALFIT run result (see notes) | em.IR.NIR |

GAL_RESULT_U | - | GALFIT run result (see notes) | em.opt.U |

GAL_RESULT_R | - | GALFIT run result (see notes) | em.opt.R |

GAL_RESULT_K | - | GALFIT run result (see notes) | em.IR.K |

GAL_RESULT_J | - | GALFIT run result (see notes) | em.IR.J |

GAL_RESULT_I | - | GALFIT run result (see notes) | em.opt.I |

GAL_RESULT_H | - | GALFIT run result (see notes) | em.IR.H |

GAL_RESULT_G | - | GALFIT run result (see notes) | em.opt |

GAL_RA_Z | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt |

GAL_RA_Y | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.NIR |

GAL_RA_U | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt.U |

GAL_RA_R | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt.R |

GAL_RA_K | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.K |

GAL_RA_J | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.J |

GAL_RA_I | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt.I |

GAL_RA_H | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.IR.H |

GAL_RA_G | deg | Right Ascension as determined by GALFIT | pos.eq.ra;meta.modelled;em.opt |

GAL_R90_Z | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt |

GAL_R90_Y | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.NIR |

GAL_R90_U | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt.U |

GAL_R90_R | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt.R |

GAL_R90_K | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.K |

GAL_R90_J | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.J |

GAL_R90_I | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt.I |

GAL_R90_H | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.IR.H |

GAL_R90_G | arcsec | rad containing 90% of total light (sma) | phys.angSize;meta.modelled;em.opt |

GAL_QFLAG_Z | - | quality flag (see notes) | meta.code.qual;em.opt |

GAL_QFLAG_Y | - | quality flag (see notes) | meta.code.qual;em.IR.NIR |

GAL_QFLAG_U | - | quality flag (see notes) | meta.code.qual;em.opt.U |

GAL_QFLAG_R | - | quality flag (see notes) | meta.code.qual;em.opt.R |

GAL_QFLAG_K | - | quality flag (see notes) | meta.code.qual;em.IR.K |

GAL_QFLAG_J | - | quality flag (see notes) | meta.code.qual;em.IR.J |

GAL_QFLAG_I | - | quality flag (see notes) | meta.code.qual;em.opt.I |

GAL_QFLAG_H | - | quality flag (see notes) | meta.code.qual;em.IR.H |

GAL_QFLAG_G | - | quality flag (see notes) | meta.code.qual;em.opt |

GAL_PA_Z | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt |

GAL_PA_Y | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.NIR |

GAL_PA_U | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt.U |

GAL_PA_R | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt.R |

GAL_PA_K | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.K |

GAL_PA_J | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.J |

GAL_PA_I | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt.I |

GAL_PA_H | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.IR.H |

GAL_PA_G | deg | position angle (x+, CCW) (see notes) | pos.posAng;meta.modelled;em.opt |

GAL_PA_ERR_Z | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_Y | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_U | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_R | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_K | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_J | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_I | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_H | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_PA_ERR_G | deg | GALFIT error on position angle | pos.posAng;stat.error;meta.modelled;e... |

GAL_MU_E_Z | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_E_Y | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.NIR |

GAL_MU_E_U | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt.U |

GAL_MU_E_R | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt.R |

GAL_MU_E_K | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.K |

GAL_MU_E_J | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.J |

GAL_MU_E_I | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt.I |

GAL_MU_E_H | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.IR.H |

GAL_MU_E_G | mag/arcsec^2 | effective surface brightness at re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_E_AVG_Z | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_E_AVG_Y | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.NIR |

GAL_MU_E_AVG_U | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt.U |

GAL_MU_E_AVG_R | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt.R |

GAL_MU_E_AVG_K | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.K |

GAL_MU_E_AVG_J | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.J |

GAL_MU_E_AVG_I | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt.I |

GAL_MU_E_AVG_H | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.IR.H |

GAL_MU_E_AVG_G | mag/arcsec^2 | effective surface brightness within re | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_0_Z | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt |

GAL_MU_0_Y | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.NIR |

GAL_MU_0_U | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt.U |

GAL_MU_0_R | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt.R |

GAL_MU_0_K | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.K |

GAL_MU_0_J | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.J |

GAL_MU_0_I | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt.I |

GAL_MU_0_H | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.IR.H |

GAL_MU_0_G | mag/arcsec^2 | central surface brightness | phot.mag.sb;meta.modelled;em.opt |

GAL_MAG_Z | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt |

GAL_MAG_Y | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.NIR |

GAL_MAG_U | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt.U |

GAL_MAG_R | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt.R |

GAL_MAG_K | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.K |

GAL_MAG_J | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.J |

GAL_MAG_I | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt.I |

GAL_MAG_H | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.IR.H |

GAL_MAG_G | mag | magnitude of Sersic model | phot.mag;meta.modelled;em.opt |

GAL_MAG_ERR_Z | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.opt |

GAL_MAG_ERR_Y | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.... |

GAL_MAG_ERR_U | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.... |

GAL_MAG_ERR_R | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.... |

GAL_MAG_ERR_K | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.... |

GAL_MAG_ERR_J | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.... |

GAL_MAG_ERR_I | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.... |

GAL_MAG_ERR_H | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.... |

GAL_MAG_ERR_G | mag | GALFIT error on magnitude | phot.mag;stat.error;meta.modelled;em.opt |

GAL_MAG_10RE_Z | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt |

GAL_MAG_10RE_Y | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.NIR |

GAL_MAG_10RE_U | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt.U |

GAL_MAG_10RE_R | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt.R |

GAL_MAG_10RE_K | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.K |

GAL_MAG_10RE_J | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.J |

GAL_MAG_10RE_I | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt.I |

GAL_MAG_10RE_H | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.IR.H |

GAL_MAG_10RE_G | mag | magnitude of model, truncated at 10*re | phot.mag;meta.modelled;em.opt |

GAL_ITERATIONS_Z | - | number of iterations for convergence | meta.number;em.opt |

GAL_ITERATIONS_Y | - | number of iterations for convergence | meta.number;em.IR.NIR |

GAL_ITERATIONS_U | - | number of iterations for convergence | meta.number;em.opt.U |

GAL_ITERATIONS_R | - | number of iterations for convergence | meta.number;em.opt.R |

GAL_ITERATIONS_K | - | number of iterations for convergence | meta.number;em.IR.K |

GAL_ITERATIONS_J | - | number of iterations for convergence | meta.number;em.IR.J |

GAL_ITERATIONS_I | - | number of iterations for convergence | meta.number;em.opt.I |

GAL_ITERATIONS_H | - | number of iterations for convergence | meta.number;em.IR.H |

GAL_ITERATIONS_G | - | number of iterations for convergence | meta.number;em.opt |

GAL_INDEX_Z | - | Sersic index | stat.fit.param;meta.modelled;em.opt |

GAL_INDEX_Y | - | Sersic index | stat.fit.param;meta.modelled;em.IR.NIR |

GAL_INDEX_U | - | Sersic index | stat.fit.param;meta.modelled;em.opt.U |