The connection between galaxies and their dark matter halos
RH Wechsler, JL Tinker - Annual Review of Astronomy and …, 2018 - annualreviews.org
In our modern understanding of galaxy formation, every galaxy forms within a dark matter
halo. The formation and growth of galaxies over time is connected to the growth of the halos …
halo. The formation and growth of galaxies over time is connected to the growth of the halos …
Physical properties and environments of nearby galaxies
MR Blanton, J Moustakas - Annual Review of Astronomy and …, 2009 - annualreviews.org
We review the physical properties of nearby, relatively luminous galaxies, using results from
newly available massive data sets together with more detailed observations. First, we …
newly available massive data sets together with more detailed observations. First, we …
The DEEP2 galaxy redshift survey: Design, observations, data reduction, and redshifts
We describe the design and data analysis of the DEEP2 Galaxy Redshift Survey, the
densest and largest high-precision redshift survey of galaxies at z∼ 1 completed to date …
densest and largest high-precision redshift survey of galaxies at z∼ 1 completed to date …
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 …
Galaxy bimodality due to cold flows and shock heating
A Dekel, Y Birnboim - Monthly notices of the royal astronomical …, 2006 - academic.oup.com
We address the origin of the robust bimodality observed in galaxy properties about a
characteristic stellar mass∼ 3× 1010 M⊙. Less massive galaxies tend to be ungrouped …
characteristic stellar mass∼ 3× 1010 M⊙. Less massive galaxies tend to be ungrouped …
The reversal of the star formation-density relation in the distant universe
Aims. We study the relationship between the local environment of galaxies and their star
formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at. Methods …
formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at. Methods …
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 …
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 …
The herschel atlas
The Herschel ATLAS is the largest open-time key project that will be carried out on the
Herschel Space Observatory. It will survey 570 deg 2 of the extragalactic sky, 4 times larger …
Herschel Space Observatory. It will survey 570 deg 2 of the extragalactic sky, 4 times larger …
Galaxy bimodality versus stellar mass and environment
Abstract We analyse az< 0.1 galaxy sample from the Sloan Digital Sky Survey focusing on
the variation in the galaxy colour bimodality with stellar mass and projected neighbour …
the variation in the galaxy colour bimodality with stellar mass and projected neighbour …