3.3.13.6  :  All Sky Map Tables

An all sky lightcone created using the Bruzual & Charlot (2003) stellar populations resides in the table wmap1.BC03_AllSky_001. It was constructed by replicating the Millennium simulation box (500Mpc/h on a side) with no additional transformations applied. The catalogue is limited to an apparent observer-frame AB magnitude of i< 21.0 and includes apparent observer-frame magnitudes for 9 filters: SDSS u, g, r, i, z and VISTA Y, J, H, Ks. The algorithm is equivalent to the one used for the all sky map in MPAMocks..Blaizot2006_AllSky_PT_1.

namedatatypeunitUCDdescription
GalIDbigint[ucd]Identifier of the galaxy in the Guo2010a..MR table. Pointer to the galaxyId column in that table.
HaloIDbigint[ucd]Identifier of the halo (in the MPHalotrees..MHalo table) that this galaxy resides in. Pointer to the haloId column in that table.
cxrealMpc/h[ucd]X-component of galaxy's position in 3D space. Origin of coordinate system is at the origin of the cone. The coordinate axes are aligned with those of the simulation box which is supposed to be periodically extended
cyrealMpc/h[ucd]Y-component of galaxy's position in 3D space. Origin of coordinate system is at the origin of the cone. The coordinate axes are aligned with those of the simulation box which is supposed to be periodically extended.
czrealMpc/h[ucd]Z-component of galaxy's position in 3D space. Origin of coordinate system is at the origin of the cone. The coordinate axes are aligned with those of the simulation box which is supposed to be periodically extended.
rarealdeg[ucd]Right ascension, i.e. longitude component of the galaxy's position on the sky. Assumed that center of cone is at RA=0.
decrealdeg[ucd]Declination, i.e. latitude component of the galaxy's position on the sky. Assumed that center of cone is at Dec=0.
z_georeal[ucd]Redshift of the galaxy based on its position. Peculiar velocity is not included.
z_appreal[ucd]Apparent redshift. Including peculiar velocity.
dlumrealMpc/h[ucd]Luminosity distance in Mpc/h.
vlosrealkm/s[ucd]Line-of-sight velocity of the galaxy in km/s.
inclrealdeg[ucd]Inclination of the galaxy. Randomly generated and used in the galaxy formation algorithms to perform dust correction on the luminosities.
SDSS_ureal[ucd]Observer-frame apparent (AB) magnitude in the SDSS u filter (dust corrected) of the galaxy.
SDSS_greal[ucd]Observer-frame apparent (AB) magnitude in the SDSS g filter (dust corrected) of the galaxy.
SDSS_rreal[ucd]Observer-frame apparent (AB) magnitude in the SDSS r filter (dust corrected) of the galaxy.
SDSS_ireal[ucd]Observer-frame apparent (AB) magnitude in the SDSS i filter (dust corrected) of the galaxy.
SDSS_zreal[ucd]Observer-frame apparent (AB) magnitude in the SDSS z filter (dust corrected) of the galaxy.
Yreal[ucd]Observer-frame apparent (AB) magnitude in the VISTA Y filter (dust corrected) of the galaxy.
Jreal[ucd]Observer-frame apparent (AB) magnitude in the VISTA/2MASS J filter (dust corrected) of the galaxy.
Hreal[ucd]Observer-frame apparent (AB) magnitude in the VISTA/2MASS H filter (dust corrected) of the galaxy.
Ksreal[ucd]Observer-frame apparent (AB) magnitude in the VISTA/2MASS Ks filter (dust corrected) of the galaxy.
SDSS_u_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the SDSS u filter (dust corrected) of the bulge.
SDSS_g_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the SDSS g filter (dust corrected) of the bulge.
SDSS_r_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the SDSS r filter (dust corrected) of the bulge.
SDSS_i_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the SDSS i filter (dust corrected) of the bulge.
SDSS_z_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the SDSS z filter (dust corrected) of the bulge.
Y_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the VISTA Y filter (dust corrected) of the bulge.
J_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the VISTA/2MASS J filter (dust corrected) of the bulge.
H_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the VISTA/2MASS H filter (dust corrected) of the bulge.
Ks_Bulgereal[ucd]Observer-frame apparent (AB) magnitude in the VISTA/2MASS Ks filter (dust corrected) of the bulge.