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28 March 2024
 
  » arxiv » astro-ph/0012105

 Article overview


The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey III: The Power Spectrum
Peter Schuecker ; Hans Boehringer ; Luigi Guzzo ; Chris A. Collins ; Doris M. Neumann ; Sabine Schindler ; Wolfgang Voges ; Sabrina De Grandi ; Guido Chincarini ; Ray Cruddace ; Volker Mueller ; Thomas H. Reiprich ; Joerg Retzlaff ; Peter Shaver ;
Date 5 Dec 2000
Subject astro-ph
AbstractWe present a measure of the power spectrum on scales from 15 to 800 Mpc/h using the ROSAT-ESO Flux-Limited X-Ray(REFLEX) galaxy cluster catalogue. The REFLEX survey provides a sample of the 452 X-ray brightest southern clusters of galaxies with the nominal flux limit S=3.0 10^{-12}erg/s/cm2 for the ROSAT energy band (0.1-2.4)keV. Several tests are performed showing no significant incompletenesses of the REFLEX clusters with X-ray luminosities brighter than 10^{43}erg/s up to scales of about 800 Mpc/h. They also indicate that cosmic variance might be more important than previous studies suggest. We regard this as a warning not to draw general cosmological conclusions from cluster samples with a size smaller than REFLEX. Power spectra, P(k), of comoving cluster number densities are estimated for flux- and volume-limited subsamples. The most important result is the detection of a broad maximum within the comoving wavenumber range 0.022
Source arXiv, astro-ph/0012105
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