The many flavours of photometric redshifts
Since more than 70 years ago, the colours of galaxies derived from flux measurements at
different wavelengths have been used to estimate their cosmological distances. Such …
different wavelengths have been used to estimate their cosmological distances. Such …
Stellar population diagnostics of elliptical galaxy formation
A Renzini - Annu. Rev. Astron. Astrophys., 2006 - annualreviews.org
Major progress has been achieved in recent years in mapping the properties of passively-
evolving, early-type galaxies (ETG) from the local universe all the way to redshift∼ 2. Here …
evolving, early-type galaxies (ETG) from the local universe all the way to redshift∼ 2. Here …
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 …
UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
HJ McCracken, B Milvang-Jensen, J Dunlop… - Astronomy & …, 2012 - aanda.org
In this paper we describe the first data release of the UltraVISTA near-infrared imaging
survey of the COSMOS field. We summarise the key goals and design of the survey and …
survey of the COSMOS field. We summarise the key goals and design of the survey and …
[图书][B] Galaxy formation and evolution
The rapidly expanding field of galaxy formation lies at the interface between astronomy,
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …
The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies
We use a complete sample of galaxies drawn from the Sloan Digital Sky Survey to study
how structure, star formation and nuclear activity depend on local density and on stellar …
how structure, star formation and nuclear activity depend on local density and on stellar …
The SINS survey: SINFONI integral field spectroscopy of z∼ 2 star-forming galaxies
NMF Schreiber, R Genzel, N Bouché… - The Astrophysical …, 2009 - iopscience.iop.org
ABSTRACT We present the Spectroscopic Imaging survey in the near-infrared (near-IR) with
SINFONI (SINS) of high-redshift galaxies. With 80 objects observed and 63 detected in at …
SINFONI (SINS) of high-redshift galaxies. With 80 objects observed and 63 detected in at …
Nearly 5000 distant early-type galaxies in COMBO-17: a red sequence and its evolution since z~ 1
We present the rest-frame colors and luminosities of~ 25,000 m R≲ 24 galaxies in the
redshift range 0.2< z≤ 1.1 drawn from 0.78 deg 2 of the COMBO-17 survey (Classifying …
redshift range 0.2< z≤ 1.1 drawn from 0.78 deg 2 of the COMBO-17 survey (Classifying …
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 VIMOS Ultra-Deep Survey:~ 10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2< z≃ 6
O Le Fèvre, LAM Tasca, P Cassata, B Garilli… - Astronomy & …, 2015 - aanda.org
We present the VIMOS Ultra Deep Survey (VUDS), a spectroscopic redshift survey of~ 10
000 very faint galaxies to study the main phase of galaxy assembly in 2< z≃ 6. The survey …
000 very faint galaxies to study the main phase of galaxy assembly in 2< z≃ 6. The survey …