Generate grids of SPS models for redshifts outside the range of interest (i.e. for 0 < z < 1 and 2.5 < z < 3) and the same range of SP ages, starburst durations, galaxy metallicity and observational S/N that as used for the models in the interesting redshift range (1 < z < 2.5).
These models can be used to determine the degree of contamination of any sample selected based on redshifts derived using the fitting procedure under test.
hughdickinson
commented
7 years ago
Generate grids of SPS models for redshifts outside the range of interest (i.e. for 0 < z < 1 and 2.5 < z < 3) and the same range of SP ages, starburst durations, galaxy metallicity and observational S/N that as used for the models in the interesting redshift range (1 < z < 2.5).
These models can be used to determine the degree of contamination of any sample selected based on redshifts derived using the fitting procedure under test.