Ram pressure strip** in high-density environments
Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
[HTML][HTML] Numerical simulations of the dark universe: State of the art and the next decade
M Kuhlen, M Vogelsberger, R Angulo - Physics of the Dark Universe, 2012 - Elsevier
We present a review of the current state of the art of cosmological dark matter simulations,
with particular emphasis on the implications for dark matter detection efforts and studies of …
with particular emphasis on the implications for dark matter detection efforts and studies of …
The COSMOS2015 galaxy stellar mass function-Thirteen billion years of stellar mass assembly in ten snapshots
I Davidzon, O Ilbert, C Laigle, J Coupon… - Astronomy & …, 2017 - aanda.org
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 …
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …
The BAHAMAS project: calibrated hydrodynamical simulations for large-scale structure cosmology
IG McCarthy, J Schaye, S Bird… - Monthly Notices of the …, 2016 - academic.oup.com
The evolution of the large-scale distribution of matter is sensitive to a variety of fundamental
parameters that characterise the dark matter, dark energy, and other aspects of our …
parameters that characterise the dark matter, dark energy, and other aspects of our …
A unified multiwavelength model of galaxy formation
We present a new version of the galform semi-analytical model of galaxy formation. This
brings together several previous developments of galform into a single unified model …
brings together several previous developments of galform into a single unified model …
The origin and evolution of the galaxy mass–metallicity relation
X Ma, PF Hopkins, CA Faucher-Giguère… - Monthly Notices of …, 2016 - academic.oup.com
We use high-resolution cosmological zoom-in simulations from the Feedback in Realistic
Environment (FIRE) project to study the galaxy mass–metallicity relations (MZR) from z= 0 …
Environment (FIRE) project to study the galaxy mass–metallicity relations (MZR) from z= 0 …
A redshift-independent efficiency model: star formation and stellar masses in dark matter halos at z≳ 4
S Tacchella, S Bose, C Conroy… - The Astrophysical …, 2018 - iopscience.iop.org
We explore the connection between the UV luminosity functions (LFs) of high-z galaxies and
the distribution of stellar masses and star formation histories (SFHs) in their host dark matter …
the distribution of stellar masses and star formation histories (SFHs) in their host dark matter …
The Hydrangea simulations: galaxy formation in and around massive clusters
YM Bahé, DJ Barnes, C Dalla Vecchia… - Monthly Notices of …, 2017 - academic.oup.com
We introduce the Hydrangea simulations, a suite of 24 cosmological hydrodynamic zoom-in
simulations of massive galaxy clusters (M 200c= 1014–1015.4 M⊙) with baryon particle …
simulations of massive galaxy clusters (M 200c= 1014–1015.4 M⊙) with baryon particle …
Ancient light from young cosmic cities: physical and observational signatures of galaxy proto-clusters
YK Chiang, R Overzier, K Gebhardt - The Astrophysical Journal, 2013 - iopscience.iop.org
ABSTRACT A growing number of galaxy clusters at z= 1–2 is being discovered as part of
deep optical, IR, X-ray, and Sunyaev–Zel'dovich effect surveys. For a complete picture of …
deep optical, IR, X-ray, and Sunyaev–Zel'dovich effect surveys. For a complete picture of …
Bulge Growth and Quenching since z= 2.5 in CANDELS/3D-HST
P Lang, S Wuyts, RS Somerville… - The Astrophysical …, 2014 - iopscience.iop.org
Exploiting the deep high-resolution imaging of all five CANDELS fields, and accurate
redshift information provided by 3D-HST, we investigate the relation between structure and …
redshift information provided by 3D-HST, we investigate the relation between structure and …