The stellar masses, mean ages, metallicities, and star formation histories of galaxies are
now commonly estimated via stellar population synthesis (SPS) techniques. SPS relies on …

We develop a model for the cosmological role of mergers in the evolution of starbursts,
quasars, and spheroidal galaxies. By combining theoretically well-constrained halo and …

We present a new semi-analytic model that self-consistently traces the growth of
supermassive black holes (BH) and their host galaxies within the context of the Lambda cold …

We estimate the galaxy stellar mass function and stellar mass density for star-forming and
quiescent galaxies with 0.2< z< 4. We construct a large, deep (K s< 24) sample of 220 000 …

We measure the evolution of the stellar mass function (SMF) from z= 0–1 using multi-
wavelength imaging and spectroscopic redshifts from the PRism MUlti-object Survey …

We compare the predictions of Horizon-AGN, a hydrodynamical cosmological simulation
that uses an adaptive mesh refinement code, to observational data in the redshift range 0< …

We use a modified version of the halo-based group finder developed by Yang et al. to select
galaxy groups from the Sloan Digital Sky Survey (SDSS DR4). In the first step, a combination …

The DEEP2 and COMBO-17 surveys are compared to study luminosity functions of red and
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but …

GALAXY STELLAR MASS ASSEMBLY BETWEEN 0.2 < z < 2 FROM THE S-COSMOS
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We present the galaxy stellar mass function (GSMF) to redshift z≃ 1, based on the analysis
of about 8500 galaxies with I< 22.5 (AB mag) over 1.4 deg 2, which are part of the …