HIGHLIGHTS
SUMMARY
In this framework, the study of galaxy clusters at different redshifts is key to understanding the role of the environment in the evolution, or transition, from star forming galaxies (SFGs) to red and passive galaxies (Alberts et_al 2016). On one hand, in the local Universe, and up to z ~ 1.4, the dense cores of galaxy clusters are preferentially populated by massive early-type galaxies that form a tight sequence in the color-magnitude diagram (CMD), the so-called red sequence (Bell et_al 2004). Alberts et_al, studying SF and AGN activity in 11 galaxy . . .
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