HIGHLIGHTS
SUMMARY
The shape of the MSR is consistent with a scenario in which galaxy growth is dominated by star formation due to cold gas accretion up to a certain mass (which is redshift- and sizedependent, corresponding to M=1011 M at z=2 and Re=1 kpc approximately) and by galaxy mergers at higher masses (e_g, Shankar et_al 2013; van Dokkum et_al 2015; Zanisi et_al 2020) Is the same for galaxies in the field and dense environments (e_g, Rettura et_al 2010; Huertas-Company et_al 2013a; Kelkar et_al 2015; Saracco et_al 2017), and for stellar mass . . .
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