LoCuSS: Probing galaxy transformation physics with Herschel

Astronomy and Astrophysics

Volumn 518, Issue 7-8, 2010, Pages

  Smith, G P ^a   Haines, C P ^a   Pereira, M J ^b   Egami, E ^b   Moran, S M ^c   Hardegree Ullman, E ^d   Babul, A ^e   Rex, M ^b   Rawle, T D ^b   Zhang, Y Y ^f   Finoguenov, A ^g,h   Okabe, N ⁱ   Sanderson, A J R ^a   Edge, A C ^j   Takada, M ^k  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b UNIVERSITY OF ARIZONA   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d RENSSELAER POLYTECHNIC INSTITUTE   (United States)

^e UNIVERSITY OF VICTORIA   (Canada)

^f UNIVERSITY OF BONN   (Germany)

^g MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^h NATIONAL SPACE SCIENCE AND TECHNOLOGY CENTER   (United States)

ⁱ INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^j DURHAM UNIVERSITY   (United Kingdom)

^k UNIVERSITY OF TOKYO   (Japan)

more..

Author keywords

Galaxies: clusters: general; Galaxies: star formation; Galaxy: evolution; Infrared: galaxies

Indexed keywords

ION BEAMS; LUMINANCE; SIZE DISTRIBUTION; SYSTEMATIC ERRORS;

CLUSTER CENTERS; CLUSTER CORES; CLUSTER MASS; CLUSTER MASS DISTRIBUTIONS; FLUX RATIO; FORMATION RATES; GALAXIES: CLUSTERS: GENERAL; GALAXIES: STAR FORMATION; GALAXY CLUSTERS; GALAXY: EVOLUTION; HERSCHEL; HIERARCHICAL ASSEMBLIES; INFRARED LUMINOSITY; INFRARED: GALAXIES; MASS FUNCTIONS; MULTIWAVELENGTH; RAM-PRESSURE STRIPPING; SPATIAL DISTRIBUTION; STAR FORMING GALAXY;

GALAXIES;

EID: 77957851684     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014691     Document Type: Article

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