This overview paper describes the legacy prospect and discovery potential of the Dark
Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the …

Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …

We present new stellar mass functions at z∼ 6, z∼ 7, z∼ 8, z∼ 9 and, for the first time, z∼
10, constructed from∼ 800 Lyman-break galaxies previously identified over the eXtreme …

Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …

Broadband photometry of galaxies measures an unresolved mix of complex stellar
populations, gas, and dust. Interpreting these data is a challenge for models: many studies …

We present emerge, an E mpirical M od E l for the fo R mation of G alaxi E s, describing the
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …

We measure the stellar mass function (SMF) and stellar mass density of galaxies in the
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …

We constrain the slope of the star formation rate (SFR; log Ψ) to stellar mass (log M⋆)
relation down to log (M⋆/M☉)= 8.4 (log (M⋆/M☉)= 9.2) at z= 0.5 (z= 2.5) with a mass …

ABSTRACT The 3D-HST and CANDELS programs have provided WFC3 and ACS
spectroscopy and photometry over≈ 900 arcmin 2 in five fields: AEGIS, COSMOS, GOODS …

We have updated the Munich galaxy formation model to the Planck first-year cosmology,
while modifying the treatment of baryonic processes to reproduce recent data on the …