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Galaxy formation in the Planck cosmology – I. Matching the observed evolution of star formation rates, colours and stellar masses
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 …
while modifying the treatment of baryonic processes to reproduce recent data on the …
Galaxy evolution in groups and clusters: satellite star formation histories and quenching time-scales in a hierarchical Universe
AR Wetzel, JL Tinker, C Conroy… - Monthly Notices of the …, 2013 - academic.oup.com
Satellite galaxies in groups and clusters are more likely to have low star formation rates
(SFRs) and lie on the 'red sequence'than central ('field') galaxies. Using galaxy group/cluster …
(SFRs) and lie on the 'red sequence'than central ('field') galaxies. Using galaxy group/cluster …
The Aquarius Project: the subhaloes of galactic haloes
We have performed the largest ever particle simulation of a Milky Way sized dark matter
halo, and present the most comprehensive convergence study for an individual dark matter …
halo, and present the most comprehensive convergence study for an individual dark matter …
Mass assembly in quiescent and star-forming galaxies since z≃ 4 from UltraVISTA
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 …
quiescent galaxies with 0.2< z< 4. We construct a large, deep (K s< 24) sample of 220 000 …
The galaxy stellar mass function at 3.5≤ z≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields
A Grazian, A Fontana, P Santini, JS Dunlop… - Astronomy & …, 2015 - aanda.org
Context. The form and evolution of the galaxy stellar mass function (GSMF) at high redshifts
provide crucial information on star formation history and mass assembly in the young …
provide crucial information on star formation history and mass assembly in the young …
Tracing the quenching journey across cosmic time
G De Lucia, F Fontanot, L **e… - Astronomy & …, 2024 - aanda.org
We present the latest version of the GAlaxy Evolution and Assembly (GAEA) theoretical
model of galaxy formation. Our new model now combines (i) an updated treatment of …
model of galaxy formation. Our new model now combines (i) an updated treatment of …
zCOSMOS–10k-bright spectroscopic sample-the bimodality in the galaxy stellar mass function: exploring its evolution with redshift
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 …
of about 8500 galaxies with I< 22.5 (AB mag) over 1.4 deg 2, which are part of the …
Galaxy formation in WMAP1 and WMAP7 cosmologies
Using the technique of Angulo & White, we scale the Millennium and Millennium II
simulations of structure growth in a Λ cold dark matter (ΛCDM) universe from the …
simulations of structure growth in a Λ cold dark matter (ΛCDM) universe from the …
The environmental history of group and cluster galaxies in a Λ cold dark matter universe
We use publicly available galaxy merger trees, obtained applying semi-analytic techniques
to a large high-resolution cosmological simulation, to study the environmental history of …
to a large high-resolution cosmological simulation, to study the environmental history of …
The evolution of the stellar mass function of galaxies from z= 4.0 and the first comprehensive analysis of its uncertainties: evidence for mass-dependent evolution
D Marchesini, PG Van Dokkum… - The Astrophysical …, 2009 - iopscience.iop.org
We present the evolution of the stellar mass function (SMF) of galaxies from z= 4.0 to z= 1.3
measured from a sample constructed from the deep near-infrared Multi-wavelength Survey …
measured from a sample constructed from the deep near-infrared Multi-wavelength Survey …