#  The density of objects with successful redshifts for a specific target class
# (such as LRG) will be nobs*success (for example, nobs_lrg*success_lrg).
# The redshift distributions in the nz_*.dat files should be normalized
# to these number densities.

area: 14000. # full survey sky area in sq deg

ntarget_lrg:  350. # LRG targets to tile
ntarget_elg: 3000. # ELG targets to tile
ntarget_qso:  140. # QSO targets to tile, all redshifts
ntarget_lya:   45. # Lyman-alpha QSO targets to tile, z > 2.1
ntarget_badqso:  110. # Bad QSO targets (stars) to tile

nobs_lrg:  350. # observed LRG targets per sq deg
nobs_elg: 2190. # observed ELG targets per sq deg (73% of 3000)
nobs_qso:  140. # observed QSO targets per sq deg, all redshifts
nobs_lya:   45. # observed Lyman-alpha QSO targets per sq deg, z > 2.1

success_lrg: 0.86 # fraction of LRGs with successful redshift
success_elg: 0.75 # fraction of ELGs with successful redshift
success_qso: 1.00 # fraction of QSOs with successful redshift
success_lya: 1.00 # fraction of Lyman-alpha QSOs with successful redshift