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cosmos_info.header
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#
# Release of the COSMOS Mock Catalogue
# July 2011
#
##########################################
# PEOPLE
#
# Photo-z catalogue from O. Ilbert
#
# Magnitude computation from S. Jouvel
#
# Emission line computation from J. Zoubian
# Spectroscopic data used for it
# from the zCOSMOS team (PI S. Lilly), F. Lamareille
#
#
##########################################
# SELECTION OF THE CATALOGUE
#
# The catalog contain only galaxy matched with ACS data.
#
# Total number of objects: 536 983
#
#############################################
### HEADER
#############################################
#
# Object identification
#
# 1 Id Identifier
#
#############################################
#
# Best fit obtained with the galaxy templates
#
# 2 type Object type: 1=galaxy ; 2=agn ; 3=star
# 3 Mod Best fit template (1->8 Ell-S0, 9->15 Sa-Sc, 16->19 Sd-Sdm,>=20 SB)
# 4 z Redshift
# 5 E(B-V) Color
# 6 DMz Distance modulus (assume lambdaCDM comology with H0=70, om0:0.3, l0=0.7)
#
#############################################
#
# Physical properties derived from the BC03 best-fit templates at zPDF
# (Chabrier IMF, templates described in Ilbert et al. 2009, mass function paper).
# The fit are preformed only with the broad bands and without IR prior to save computational time
# (different from the mass function paper)
#
# 7 MNUV Absolute magnitudes NUV galex
# 8 Mstar log of stellar mass
#
#############################################
#
# Additional information
#
# 9 half_light_radius Half light radius in pixel (0.03 arcsec/pix) from Leauthaud et al. 2009
# 10 ROII [OII] lines ratio (OII3726/OII3729)
#
#############################################
#
# Simulation data
#
# 11 [3] Mapp_* Apparente magnitude in band *
# 12 [3] Ran_* Apparent magnitude randomized according to the error in band *
# 13 [3] Err_* Errors on magnitude in band *
# Computed magnitudes:
# U_CFHT
# B_subaru,V_subaru,g_subaru,r_subaru,i_subaru,z_subaru,
# J_WFCAM,
# H_WIRCAM,K_WIRCAM,
# F814W (HST),
# IRAC_CH1,IRAC_CH2,IRAC_CH3,IRAC_CH4,
# FUV,NUV, (galex)
#
# 102 [4] Lambda_* Wavelenght of line * (in observer referencial) [Angstrom]
# 103 [4] Flux_* Flux in line * [erg/s/cm2]
# 104 [4] Conti_* Flux in continium under the line * [erg/s/cm2/Hz]
# 105 [4] Disp_* Width of the line (sigma of the Gaussian profile
# Computed emission lines:
# Balmer Lines (Ly, Hb, Hd, Hg, Ha)
# Oxygen Lines (OII, OIIIa, OIIIb)
# Nitrogen Line (NII)
# Sulfur Lines (SIIa, SIIb)
#
# Note: all magnitudes are AB normalized.