The scaling relation between richness and mass of galaxy clusters: A Bayesian approach

Monthly Notices of the Royal Astronomical Society

Volumn 404, Issue 4, 2010, Pages 1922-1937

  Andreon, S ^a   Hurn, M A ^b  

^a INAF IASF MILANO   (Italy)

^b University of Bath   (United Kingdom)

Author keywords

Cosmological parameters; Galaxies: clusters: general; Galaxies: elliptical and lenticular, cD; Galaxies: luminosity function, mass function; Methods: statistical; X rays: galaxies: clusters

Indexed keywords

BAYESIAN NETWORKS; DISPERSIONS; LUMINANCE; STOCHASTIC SYSTEMS; SURVEYS; UNCERTAINTY ANALYSIS;

CLUSTER MASS; COSMOLOGICAL PARAMETERS; GALAXIES: CLUSTERS: GENERAL; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXIES: LUMINOSITY FUNCTION; GALAXY: LUMINOSITY FUNCTION, MASS FUNCTION; MASS FUNCTIONS; METHODS:STATISTICAL; VELOCITY DISPERSION; X-RAYS GALAXIES CLUSTERS;

GALAXIES;

EID: 77953547668     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16406.x     Document Type: Article

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