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Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

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arxiv 0801.4380 v2 pith:DCU643VC submitted 2008-01-29 astro-ph

Tommaso Giannantonio (ICG Portsmouth) , Ryan Scranton (Pittsburgh) , Robert G. Crittenden (ICG Portsmouth) , Robert C. Nichol (ICG Portsmouth) , Stephen P. Boughn (Haverford) , Adam D. Myers (Illinois) , Gordon T. Richards (Drexel) This is my paper · ORCID
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We present a global measurement of the integrated Sachs-Wolfe (ISW) effect obtained by cross-correlating all relevant large scale galaxy data sets with the cosmic microwave background radiation map provided by the Wilkinson Microwave Anisotropy Probe. With these measurements, the overall ISW signal is detected at the ~ 4.5 sigma level. We also examine the cosmological implications of these measurements, particularly the dark energy equation of state w, its sound speed, and the overall curvature of the Universe. The flat LCDM model is a good fit to the data and, assuming this model, we find that the ISW data constrain Omega_m = 0.20 +0.19 -0.11 at the 95% confidence level. When we combine our ISW results with the latest baryon oscillation and supernovae measurements, we find that the result is still consistent with a flat LCDM model with w = -1 out to redshifts z > 1.

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