Speaker
Mr
Iker Millán Irigoyen
(CIEMAT)
Description
As high redshift galaxies cannot be resolved, it is necessary to have the information of the whole stellar population in order to interpret correctly the data. Thus, templates of spectra of simple stellar populations (SSPs) are needed to extract information about the stellar populations. We present our new high resolution spectra of SSPs. We have tested the application of the spectra testing the evolution of the color-color diagrams.
