Mass and Environment as Drivers of Galaxy Evolution in SDSS and zCOSMOS and the Origin of the Schechter Function
Y Peng, SJ Lilly, K Kovač, M Bolzonella…�- The Astrophysical�…, 2010 - iopscience.iop.org
We explore the simple inter-relationships between mass, star formation rate, and
environment in the SDSS, zCOSMOS, and other deep surveys. We take a purely empirical�…
environment in the SDSS, zCOSMOS, and other deep surveys. We take a purely empirical�…
[HTML][HTML] Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey
O Ilbert, S Arnouts, HJ Mccracken, M Bolzonella…�- Astronomy &�…, 2006 - aanda.org
Aims. We present and release photometric redshifts for a uniquely large and deep sample of
522286 objects with in the Canada-France Hawaii Telescope Legacy Survey�…
522286 objects with in the Canada-France Hawaii Telescope Legacy Survey�…
The COSMOS2015 Catalog: Exploring the 1< z< 6 Universe with half a million galaxies
C Laigle, HJ McCracken, O Ilbert…�- The Astrophysical�…, 2016 - iopscience.iop.org
We present the COSMOS2015 24 catalog, which contains precise photometric redshifts and
stellar masses for more than half a million objects over the 2deg 2 COSMOS field. Including�…
stellar masses for more than half a million objects over the 2deg 2 COSMOS field. Including�…
Extragalactic background light inferred from AEGIS galaxy-SED-type fractions
The extragalactic background light (EBL) is of fundamental importance both for
understanding the entire process of galaxy evolution and for γ-ray astronomy, but the overall�…
understanding the entire process of galaxy evolution and for γ-ray astronomy, but the overall�…
Mass assembly in quiescent and star-forming galaxies since z≃ 4 from UltraVISTA
O Ilbert, HJ McCracken, O Le F�vre, P Capak…�- Astronomy &�…, 2013 - aanda.org
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�…
[HTML][HTML] Galaxy luminosity functions to z~ 1 from DEEP2 and COMBO-17: implications for red galaxy formation
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�…
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but�…
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�…
Introducing the NEWHORIZON simulation: Galaxy properties with resolved internal dynamics across cosmic time
Y Dubois, R Beckmann, F Bournaud, H Choi…�- Astronomy &�…, 2021 - aanda.org
Hydrodynamical cosmological simulations are increasing their level of realism by
considering more physical processes and having greater resolution or larger statistics�…
considering more physical processes and having greater resolution or larger statistics�…
zCOSMOS: a large VLT/VIMOS redshift survey covering 0< z< 3 in the COSMOS field
SJ Lilly, O Le F�vre, A Renzini…�- The Astrophysical�…, 2007 - iopscience.iop.org
Abstract zCOSMOS is a large-redshift survey that is being undertaken in the COSMOS field
using 600 hr of observation with the VIMOS spectrograph on the 8 m VLT. The survey is�…
using 600 hr of observation with the VIMOS spectrograph on the 8 m VLT. The survey is�…
[HTML][HTML] COSMOS2020: The galaxy stellar mass function-The assembly and star formation cessation of galaxies at 0.2< z≤ 7.5
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�…
within the modern landscape of galaxy evolution studies. These processes are indelibly�…