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.
The lightcone has a circular field of view of radius 4.0 degrees.
Only galaxies with apparent magnitudes brighter than 25.0 in the observer frame
SDSS r band (column SDSS_r_obs_app in the table) and cosmological redshifts less
than z=2.5 are included.
| 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
|
| BCDM |
float |
|
- |
Band Corrected Distance Modulus = 5 log10(dL/h-1Mpc) + 25 - 2.5 log10(1+zcos)
|
| ipixel |
int |
|
- |
Pixel index
|
| 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_r_obs_app |
float |
|
- |
SDSS r-filter observed frame apparent magnitude (AB) including dust extinction
|
| DES_g_obs_app |
float |
|
- |
DECam g-filter observed frame apparent magnitude (AB) including dust extinction
|
| DES_g_rest_abs |
float |
|
- |
DECam g-filter rest frame absolute magnitude (AB) including dust extinction
|
| DES_r_obs_app |
float |
|
- |
DECam r-filter observed frame apparent magnitude (AB) including dust extinction
|
| DES_r_rest_abs |
float |
|
- |
DECam r-filter rest frame absolute magnitude (AB) including dust extinction
|
| DES_i_obs_app |
float |
|
- |
DECam i-filter observed frame apparent magnitude (AB) including dust extinction
|
| DES_i_rest_abs |
float |
|
- |
DECam i-filter rest frame absolute magnitude (AB) including dust extinction
|
| DES_z_obs_app |
float |
|
- |
DECam z-filter observed frame apparent magnitude (AB) including dust extinction
|
| DES_z_rest_abs |
float |
|
- |
DECam z-filter rest frame absolute magnitude (AB) including dust extinction
|
| DES_Y_obs_app |
float |
|
- |
DECam Y-filter observed frame apparent magnitude (AB) including dust extinction
|
| DES_Y_rest_abs |
float |
|
- |
DECam Y-filter rest frame absolute magnitude (AB) including dust extinction
|
| 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
|
