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A Detection of the Integrated Sachs-Wolfe Effect

S. P. Boughn·R. G. Crittenden
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Abstract

We have detected statistically significant correlations between the cosmic microwave background and two tracers of large-scale structure, the HEAO1 A2 full sky hard X-ray map and the NVSS 1.4 GHz, nearly full sky radio galaxy survey. The level of correlations in these maps is consistent with that predicted for the integrated Sachs-Wolfe (ISW) effect in the context of a Lambda CDM cosmological model and, therefore, provides independent evidence for a cosmological constant. A maximum likelihood fit to the amplitude of the ISW effect relative to the predicted value is 1.13 +- 0.35 (statistical error only).

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S. P. Boughn, R. G. Crittenden. 2004-04-23. A Detection of the Integrated Sachs-Wolfe Effect. https://doi.org/10.1016/j.newar.2005.01.005

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