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26 April 2024
 
  » arxiv » astro-ph/0405340

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Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters
S.W. Allen ; R.W. Schmidt ; H. Ebeling ; A.C. Fabian ; L. van Speybroeck ;
Date 18 May 2004
Journal Mon.Not.Roy.Astron.Soc. 353 (2004) 457
Subject astro-ph
AffiliationIoA Cambridge), R.W. Schmidt (Potsdam University), H. Ebeling (IfA, Hawaii), A.C. Fabian (IoA Cambridge), L. van Speybroeck (CfA
AbstractWe present constraints on the mean dark energy density, Omega_X and dark energy equation of state parameter, w_X, based on Chandra measurements of the X-ray gas mass fraction in 26 X-ray luminous, dynamically relaxed galaxy clusters spanning the redshift range 0.07-1, the same data require w_X<-0.7 at 95 per cent confidence. Similar results on the mean matter density and dark energy equation of state parameter, Omega_m=0.24pm0.04 and w_X=-1.20^{+0.24}_{-0.28}, are obtained by replacing the CMB data with standard priors on the Hubble constant and mean baryon density and assuming a flat geometry.
Source arXiv, astro-ph/0405340
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