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Nelson Padilla |
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I will present a method to select descendants of
high redshift galaxies, motivated in results from numerical
simulations. If the number density and clustering amplitude of a
sample of galaxies is known, these can be matched to a population of
dark-matter haloes at the same redshift in EPS theory or numerical
simulations. The latter can be followed to lower redshifts, where
the properties of the descendant population can be inferred. The
observational sample that shares this properties at this new
redshift can be considered as statistical descendants of the higher
z sample. Applying this method to ETG galaxies in the |