Cosmological constraints from the cluster contribution to the power spectrum of the soft X-ray background. New evidence for a low σ 8?

Monthly Notices of the Royal Astronomical Society

Volumn 344, Issue 3, 2003, Pages 951-964

  Diego, J M ^a   Sliwa, W ^b   Silk, J ^a   Barcons, X ^c  

^a Nicolaus Copernicus Astron Centre ^*  (Spain)

^b Nicolaus Copernicus Astron Centre   (United Kingdom)

^c INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

Author keywords

Cosmological parameters; Galaxies: clusters: general

Indexed keywords

COSMOLOGY; GALAXIES; SYSTEMATIC ERRORS; UNCERTAINTY ANALYSIS;

ALL-SKY SURVEY; COSMOLOGICAL PARAMETERS; GALAXIES: CLUSTERS: GENERAL; POINT-SOURCES; POWER-SPECTRA; SOFT X-RAY; UNCERTAINTY; UPPER LIMITS; X-RAY BACKGROUND; X-RAY POWER;

POWER SPECTRUM;

EID: 0142198865     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06884.x     Document Type: Article

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