Cosmological constraints from the clustering properties of the X-ray Brightest Abell-type Cluster sample

Monthly Notices of the Royal Astronomical Society

Volumn 305, Issue 4, 1999, Pages 866-874

  Borgani, S ^a   Plionis, M ^b   Kolokotronis, V ^b,c  

^a SEZIONE DI TRIESTE   (Italy)

^b NATIONAL OBSERVATORY OF ATHENS   (Greece)

^c QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

Author keywords

Cosmology: theory; Galaxies: clusters: general; Large scale structure of universe

Indexed keywords

COSMIC RAYS; MAXIMUM LIKELIHOOD; POWER SPECTRUM;

CLUSTERING PROPERTIES; COSMOLOGY: THEORY; FITTING PARAMETERS; FLUX LIMITS; GALAXIES: CLUSTERS: GENERAL; LARGE SCALE STRUCTURE OF UNIVERSE; POWER-LAW; POWER-SPECTRA; TWO-POINT CORRELATION FUNCTION; UNCERTAINTY;

COSMOLOGY;

EID: 0006180450     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02468.x     Document Type: Article

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