The environmental dependence of the stellar mass function at z ~ 1: Comparing cluster and field between the GCLASS and UltraVISTA surveys

Astronomy and Astrophysics

Volumn 557, Issue , 2013, Pages

  Van Der Burg, R F J ^a   Muzzin, A ^a   Hoekstra, H ^a   Lidman, C ^b   Rettura, A ^c   Wilson, G ^d   Yee, H K C ^e   Hildebrandt, H ^f,g   Marchesini, D ^h   Stefanon, M ⁱ   Demarco, R ^j   Kuijken, K ^a  

^a LEIDEN UNIVERSITY   (Netherlands)

^b AUSTRALIAN ASTRONOMICAL OBSERVATORY   (Australia)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e UNIVERSITY OF TORONTO   (Canada)

^f UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^g UNIVERSITY OF BONN   (Germany)

^h TUFTS UNIVERSITY   (United States)

ⁱ UNIVERSITY OF MISSOURI   (United States)

^j UNIVERSITY OF CONCEPCIÓN   (Chile)

more..

Author keywords

Galaxies: clusters: general; Galaxies: evolution; Galaxies: luminosity function, mass function; Galaxies: photometry

Indexed keywords

FALSE POSITIVE AND FALSE NEGATIVES; GALAXIES: CLUSTERS: GENERAL; GALAXIES: EVOLUTIONS; GALAXIES: PHOTOMETRY; GALAXIES:LUMINOSITY FUNCTION , MASS FUNCTION; HIGH-DENSITY ENVIRONMENT; SPECTRAL ENERGY DISTRIBUTION; SPECTROSCOPIC SURVEYS;

ASTROPHYSICS; PHOTOMETRY; QUENCHING; STARS; SURVEYS;

GALAXIES;

EID: 84882363654     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201321237     Document Type: Article

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