Photometric redshifts as a tool for studying the Coma cluster galaxy populations

Astronomy and Astrophysics

Volumn 491, Issue 3, 2008, Pages 681-692

  Adami, C ^a   Ilbert, O ^a,b   Pello R ^c   Cuillandre, J C ^d   Durret, F ^e   Mazure, A ^a   Picat, J P ^c   Ulmer, M P ^a,f  

^a OBSERVATOIRE DE MARSEILLE   (France)

^b UNIVERSITY OF HAWAII   (United States)

^c UNIVERSITÉ DE TOULOUSE   (France)

^d CANADA FRANCE HAWAII TELESCOPE   (United States)

^e INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^f NORTHWESTERN UNIVERSITY   (United States)

Author keywords

Galaxies: clusters: individual: Coma; Galaxies: luminosity function, mass function

Indexed keywords

DISTRIBUTION FUNCTIONS; GALAXIES; LUMINANCE; MOLECULAR INTERACTIONS; OPTICAL PROPERTIES; PHOTOMETRY; POPULATION STATISTICS; PROBABILITY DENSITY FUNCTION; PROBABILITY DISTRIBUTIONS; STATISTICAL METHODS;

BACKGROUND SUBTRACTIONS; CLUSTER CENTERS; CLUSTER MEMBERS; GALAXIES: CLUSTERS: INDIVIDUAL: COMA; GALAXIES: LUMINOSITY FUNCTION, MASS FUNCTION; GALAXY POPULATIONS; LATE TYPES; LUMINOSITY FUNCTIONS; PROBABILITY DISTRIBUTION FUNCTIONS; RED SHIFTS; SHORT BURSTS; SPATIAL DISTRIBUTIONS; STAR FORMATIONS; STEEP SLOPES; SUB STRUCTURES; SUBTRACTION METHODS;

VANADIUM COMPOUNDS;

EID: 57049187860     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809845     Document Type: Article

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