Only galaxies within the 5 main GAMA fields, with apparent
magnitudes brighter than 21.0 in the observer frame SDSS r band (column
SDSS_r_obs_app in the table) and cosmological redshifts less than z=0.9 are
included. The 5 main GAMA fields are numbered from 1 to 5, corresponding to
G09, G12, G15, G02 and G23 respectively, and the integer column "field" specifies
which field each galaxy in the lightcone belongs to.
The column ireal indicates which realisation of the lightcone each galaxy belongs to
and has values in the range 0 to 25.
column | type | UCD | unit | description |
UniqueGalaxyID |
string |
|
- |
Unique identifier for this periodic replication of this galaxy
|
GalaxyID |
long |
|
- |
ID of this galaxy. Each galaxy may appear more than once due to periodic replication
|
redshift_cos |
float |
|
- |
cosmological redshift of galaxy
|
redshift_obs |
float |
|
- |
observed redshift of galaxy (peculiar velocities included)
|
bulgemass |
float |
|
Msol/h |
stellar mass in bulge of galaxy
|
diskstellarmass |
float |
|
Msol/h |
stellar mass in disk of galaxy
|
coldgas |
float |
|
Msol/h |
mass of cold gas in disk of galaxy
|
type |
int |
|
- |
type/location of galaxy (0=central, 1=satellite in a subhalo, 2=satellite on a particle)
|
vdisk |
float |
|
km/s |
circular velocity of the disk at the half mass radius
|
rdisk |
float |
|
Mpc/h |
half-mass radius of disk
|
sfr |
float |
|
Msol/h/Gyr |
(instantaneous) quiescent SFR in disk
|
sfr_burst |
float |
|
Msol/h/Gyr |
SFR in bursts
|
mdhalo |
float |
|
Msol/h |
mass of the host halo (DHalo Mass)
|
UniqueDHaloID |
string |
|
- |
Unique identifier for this periodic replication of this halo
|
DHaloID |
long |
|
- |
ID of this dark matter halo. Each halo may appear more than once due to periodic replication
|
ra |
double |
|
degrees |
right ascension of galaxy
|
dec |
double |
|
degrees |
declination of galaxy
|
field |
int |
|
- |
Field index. The field number (going from 1 to 5) corresponds to G09, G12, G15, G02 and G23 respectively.
|
ireal |
int |
|
- |
Realisation index
|
BCDM |
float |
|
- |
Band Corrected Distance Modulus = 5 log10(dL/h-1Mpc) + 25 - 2.5 log10(1+zcos)
|
random |
double |
|
- |
Random number in the range 0-1
|
mag_J_obs_app |
float |
|
- |
UKIRT J-filter observed frame apparent magnitude (AB) including dust extinction
|
mag_J_rest_abs |
float |
|
- |
UKIRT J-filter rest frame absolute magnitude (AB) including dust extinction
|
mag_H_obs_app |
float |
|
- |
UKIRT H-filter observed frame apparent magnitude (AB) including dust extinction
|
mag_H_rest_abs |
float |
|
- |
UKIRT H-filter rest frame absolute magnitude (AB) including dust extinction
|
mag_K_obs_app |
float |
|
- |
UKIRT K-filter observed frame apparent magnitude (AB) including dust extinction
|
mag_K_rest_abs |
float |
|
- |
UKIRT K-filter rest frame absolute magnitude (AB) including dust extinction
|
SDSS_u_obs_app |
float |
|
- |
SDSS u-filter observed frame apparent magnitude (AB) including dust extinction
|
SDSS_u_rest_abs |
float |
|
- |
SDSS u-filter rest frame absolute magnitude (AB) including dust extinction
|
SDSS_g_obs_app |
float |
|
- |
SDSS g-filter observed frame apparent magnitude (AB) including dust extinction
|
SDSS_g_rest_abs |
float |
|
- |
SDSS g-filter rest frame absolute magnitude (AB) including dust extinction
|
SDSS_r_obs_app |
float |
|
- |
SDSS r-filter observed frame apparent magnitude (AB) including dust extinction
|
SDSS_r_rest_abs |
float |
|
- |
SDSS r-filter rest frame absolute magnitude (AB) including dust extinction
|
SDSS_i_obs_app |
float |
|
- |
SDSS i-filter observed frame apparent magnitude (AB) including dust extinction
|
SDSS_i_rest_abs |
float |
|
- |
SDSS i-filter rest frame absolute magnitude (AB) including dust extinction
|
SDSS_z_obs_app |
float |
|
- |
SDSS z-filter observed frame apparent magnitude (AB) including dust extinction
|
SDSS_z_rest_abs |
float |
|
- |
SDSS z-filter rest frame absolute magnitude (AB) including dust extinction
|
Ld_100o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_100r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_160o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_160r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_24o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_24r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_250o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_250r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_350o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_350r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_450o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_450r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_500o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_500r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_550o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_550r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_60o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_60r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_70o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_70r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_850o |
float |
|
- |
UNDOCUMENTED PROPERTY
|
Ld_850r |
float |
|
- |
UNDOCUMENTED PROPERTY
|
LBulge_Lyalpha |
float |
|
erg/s/cm2 |
Line flux for the Lyalpha line (bulge only) without dust extinction
|
LBulge_Lyalpha_ext |
float |
|
erg/s/cm2 |
Line flux for the Lyalpha line (bulge only) with dust extinction
|
LDisk_Lyalpha |
float |
|
erg/s/cm2 |
Line flux for the Lyalpha line (disk only) without dust extinction
|
LDisk_Lyalpha_ext |
float |
|
erg/s/cm2 |
Line flux for the Lyalpha line (disk only) with dust extinction
|
L_Lyalpha |
float |
|
erg/s/cm2 |
Line flux for the Lyalpha line without dust extinction
|
L_Lyalpha_ext |
float |
|
erg/s/cm2 |
Line flux for the Lyalpha line with dust extinction
|
LBulge_OII3727 |
float |
|
erg/s/cm2 |
Line flux for the OII3727 line (bulge only) without dust extinction
|
LBulge_OII3727_ext |
float |
|
erg/s/cm2 |
Line flux for the OII3727 line (bulge only) with dust extinction
|
LDisk_OII3727 |
float |
|
erg/s/cm2 |
Line flux for the OII3727 line (disk only) without dust extinction
|
LDisk_OII3727_ext |
float |
|
erg/s/cm2 |
Line flux for the OII3727 line (disk only) with dust extinction
|
L_OII3727 |
float |
|
erg/s/cm2 |
Line flux for the OII3727 line without dust extinction
|
L_OII3727_ext |
float |
|
erg/s/cm2 |
Line flux for the OII3727 line with dust extinction
|
LBulge_Hgamma |
float |
|
erg/s/cm2 |
Line flux for the Hgamma line (bulge only) without dust extinction
|
LBulge_Hgamma_ext |
float |
|
erg/s/cm2 |
Line flux for the Hgamma line (bulge only) with dust extinction
|
LDisk_Hgamma |
float |
|
erg/s/cm2 |
Line flux for the Hgamma line (disk only) without dust extinction
|
LDisk_Hgamma_ext |
float |
|
erg/s/cm2 |
Line flux for the Hgamma line (disk only) with dust extinction
|
L_Hgamma |
float |
|
erg/s/cm2 |
Line flux for the Hgamma line without dust extinction
|
L_Hgamma_ext |
float |
|
erg/s/cm2 |
Line flux for the Hgamma line with dust extinction
|
LBulge_Hbeta |
float |
|
erg/s/cm2 |
Line flux for the Hbeta line (bulge only) without dust extinction
|
LBulge_Hbeta_ext |
float |
|
erg/s/cm2 |
Line flux for the Hbeta line (bulge only) with dust extinction
|
LDisk_Hbeta |
float |
|
erg/s/cm2 |
Line flux for the Hbeta line (disk only) without dust extinction
|
LDisk_Hbeta_ext |
float |
|
erg/s/cm2 |
Line flux for the Hbeta line (disk only) with dust extinction
|
L_Hbeta |
float |
|
erg/s/cm2 |
Line flux for the Hbeta line without dust extinction
|
L_Hbeta_ext |
float |
|
erg/s/cm2 |
Line flux for the Hbeta line with dust extinction
|
LBulge_OIII4959 |
float |
|
erg/s/cm2 |
Line flux for the OIII4959 line (bulge only) without dust extinction
|
LBulge_OIII4959_ext |
float |
|
erg/s/cm2 |
Line flux for the OIII4959 line (bulge only) with dust extinction
|
LDisk_OIII4959 |
float |
|
erg/s/cm2 |
Line flux for the OIII4959 line (disk only) without dust extinction
|
LDisk_OIII4959_ext |
float |
|
erg/s/cm2 |
Line flux for the OIII4959 line (disk only) with dust extinction
|
L_OIII4959 |
float |
|
erg/s/cm2 |
Line flux for the OIII4959 line without dust extinction
|
L_OIII4959_ext |
float |
|
erg/s/cm2 |
Line flux for the OIII4959 line with dust extinction
|
LBulge_OIII5007 |
float |
|
erg/s/cm2 |
Line flux for the OIII5007 line (bulge only) without dust extinction
|
LBulge_OIII5007_ext |
float |
|
erg/s/cm2 |
Line flux for the OIII5007 line (bulge only) with dust extinction
|
LDisk_OIII5007 |
float |
|
erg/s/cm2 |
Line flux for the OIII5007 line (disk only) without dust extinction
|
LDisk_OIII5007_ext |
float |
|
erg/s/cm2 |
Line flux for the OIII5007 line (disk only) with dust extinction
|
L_OIII5007 |
float |
|
erg/s/cm2 |
Line flux for the OIII5007 line without dust extinction
|
L_OIII5007_ext |
float |
|
erg/s/cm2 |
Line flux for the OIII5007 line with dust extinction
|
LBulge_Halpha |
float |
|
erg/s/cm2 |
Line flux for the Halpha line (bulge only) without dust extinction
|
LBulge_Halpha_ext |
float |
|
erg/s/cm2 |
Line flux for the Halpha line (bulge only) with dust extinction
|
LDisk_Halpha |
float |
|
erg/s/cm2 |
Line flux for the Halpha line (disk only) without dust extinction
|
LDisk_Halpha_ext |
float |
|
erg/s/cm2 |
Line flux for the Halpha line (disk only) with dust extinction
|
L_Halpha |
float |
|
erg/s/cm2 |
Line flux for the Halpha line without dust extinction
|
L_Halpha_ext |
float |
|
erg/s/cm2 |
Line flux for the Halpha line with dust extinction
|
LBulge_NII6583 |
float |
|
erg/s/cm2 |
Line flux for the NII6583 line (bulge only) without dust extinction
|
LBulge_NII6583_ext |
float |
|
erg/s/cm2 |
Line flux for the NII6583 line (bulge only) with dust extinction
|
LDisk_NII6583 |
float |
|
erg/s/cm2 |
Line flux for the NII6583 line (disk only) without dust extinction
|
LDisk_NII6583_ext |
float |
|
erg/s/cm2 |
Line flux for the NII6583 line (disk only) with dust extinction
|
L_NII6583 |
float |
|
erg/s/cm2 |
Line flux for the NII6583 line without dust extinction
|
L_NII6583_ext |
float |
|
erg/s/cm2 |
Line flux for the NII6583 line with dust extinction
|
LBulge_CO43 |
float |
|
erg/s/cm2 |
Line flux for the CO43 line (bulge only) without dust extinction
|
LDisk_CO43 |
float |
|
erg/s/cm2 |
Line flux for the CO43 line (disk only) without dust extinction
|
LBulge_CO32 |
float |
|
erg/s/cm2 |
Line flux for the CO32 line (bulge only) without dust extinction
|
LDisk_CO32 |
float |
|
erg/s/cm2 |
Line flux for the CO32 line (disk only) without dust extinction
|
LBulge_CO21 |
float |
|
erg/s/cm2 |
Line flux for the CO21 line (bulge only) without dust extinction
|
LDisk_CO21 |
float |
|
erg/s/cm2 |
Line flux for the CO21 line (disk only) without dust extinction
|
LBulge_CO10 |
float |
|
erg/s/cm2 |
Line flux for the CO10 line (bulge only) without dust extinction
|
LDisk_CO10 |
float |
|
erg/s/cm2 |
Line flux for the CO10 line (disk only) without dust extinction
|
EW_Lyalpha |
float |
|
Angstrom |
Equivalent width of the Lyalpha line without dust extinction
|
EW_Lyalpha_ext |
float |
|
Angstrom |
Equivalent width of the Lyalpha line with dust extinction
|
EW_OII3727 |
float |
|
Angstrom |
Equivalent width of the OII3727 line without dust extinction
|
EW_OII3727_ext |
float |
|
Angstrom |
Equivalent width of the OII3727 line with dust extinction
|
EW_Hgamma |
float |
|
Angstrom |
Equivalent width of the Hgamma line without dust extinction
|
EW_Hgamma_ext |
float |
|
Angstrom |
Equivalent width of the Hgamma line with dust extinction
|
EW_Hbeta |
float |
|
Angstrom |
Equivalent width of the Hbeta line without dust extinction
|
EW_Hbeta_ext |
float |
|
Angstrom |
Equivalent width of the Hbeta line with dust extinction
|
EW_OIII4959 |
float |
|
Angstrom |
Equivalent width of the OIII4959 line without dust extinction
|
EW_OIII4959_ext |
float |
|
Angstrom |
Equivalent width of the OIII4959 line with dust extinction
|
EW_OIII5007 |
float |
|
Angstrom |
Equivalent width of the OIII5007 line without dust extinction
|
EW_OIII5007_ext |
float |
|
Angstrom |
Equivalent width of the OIII5007 line with dust extinction
|
EW_Halpha |
float |
|
Angstrom |
Equivalent width of the Halpha line without dust extinction
|
EW_Halpha_ext |
float |
|
Angstrom |
Equivalent width of the Halpha line with dust extinction
|
EW_NII6583 |
float |
|
Angstrom |
Equivalent width of the NII6583 line without dust extinction
|
EW_NII6583_ext |
float |
|
Angstrom |
Equivalent width of the NII6583 line with dust extinction
|