The observed growth of massive galaxy clusters - I. Statistical methods and cosmological constraints

Monthly Notices of the Royal Astronomical Society

Volumn 406, Issue 3, 2010, Pages 1759-1772

  Mantz, A ^a,b   Allen, S W ^a,b   Rapetti, D ^a,b   Ebeling, H ^c  

^a STANFORD UNIVERSITY   (United States)

^b SLAC NATIONAL ACCELERATOR LABORATORY   (United States)

^c UNIVERSITY OF HAWAII   (United States)

Author keywords

Cosmological parameters; Cosmology: observations; Large scale structure of Universe; X rays: galaxies: clusters

Indexed keywords

ACOUSTIC INTENSITY MEASUREMENT; COSMOLOGY; GALAXIES; HADRONS; LUMINANCE; MICROWAVE ACOUSTICS; MICROWAVE OSCILLATORS; SURVEYS;

COSMOLOGICAL PARAMETERS; COSMOLOGY OBSERVATIONS; DARK ENERGY; DATA YIELDS; EQUATION-OF-STATE; GALAXIES CLUSTERS; LARGE SCALE STRUCTURE OF UNIVERSE; SCALING RELATIONS; STATISTICAL FRAMEWORK; X-RAYS GALAXIES CLUSTERS;

SUPERNOVAE;

EID: 77955235076     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16992.x     Document Type: Article

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