This table contains galaxies in a lightcone mock catalogue based on the galaxy formation model of
Gonzalez-Perez et al.2014.
The lightcone was constructed using the technique described by
Merson et al. 2013.
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.
column | type | UCD | unit | description |
GalaxyID |
long |
|
- |
ID of this galaxy. Each galaxy may appear more than once due to periodic replication
|
UniqueGalaxyID |
string |
|
- |
Unique identifier for this periodic replication of this galaxy
|
DHaloID |
long |
|
- |
ID of this dark matter halo. Each halo may appear more than once due to periodic replication
|
UniqueDHaloID |
string |
|
- |
Unique identifier for this periodic replication of this halo
|
type |
int |
|
- |
type/location of galaxy (0=central, 1=satellite in a subhalo, 2=satellite on a particle)
|
ra |
double |
|
degrees |
right ascension of galaxy
|
dec |
double |
|
degrees |
declination of galaxy
|
redshift_cos |
float |
|
- |
cosmological redshift of galaxy
|
redshift_obs |
float |
|
- |
observed redshift of galaxy (peculiar velocities included)
|
BCDM |
float |
|
- |
Band Corrected Distance Modulus = 5 log10(dL/h-1Mpc) + 25 - 2.5 log10(1+zcos)
|
diskstellarmass |
float |
|
Msol/h |
stellar mass in disk of galaxy
|
bulgemass |
float |
|
Msol/h |
stellar mass in bulge of galaxy
|
sfr |
float |
|
Msol/h/Gyr |
(instantaneous) quiescent SFR in disk
|
sfr_burst |
float |
|
Msol/h/Gyr |
SFR in bursts
|
coldgas |
float |
|
Msol/h |
mass of cold gas in disk of galaxy
|
mdhalo |
float |
|
Msol/h |
mass of the host halo (DHalo Mass)
|
rdisk |
float |
|
Mpc/h |
half-mass radius of disk
|
vdisk |
float |
|
km/s |
circular velocity of the disk at the half mass radius
|
field |
int |
|
- |
Field index. The field number (going from 1 to 5) corresponds to G09, G12, G15, G02 and G23 respectively.
|
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
|