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An Imprint of Superstructures on the Microwave Background due to the Integrated Sachs-Wolfe Effect

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Published 2008 July 28 © 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Benjamin R. Granett et al 2008 ApJ 683 L99 DOI 10.1086/591670

1538-4357/683/2/L99

Abstract

We measure hot and cold spots on the microwave background associated with supercluster and supervoid structures identified in the Sloan Digital Sky Survey luminous red galaxy catalog. The structures give a compelling visual imprint, with a mean temperature deviation of 9.6 ± 2.2 μK, i.e., above 4 σ. We interpret this as a detection of the late-time integrated Sachs-Wolfe (ISW) effect, in which cosmic acceleration from dark energy causes gravitational potentials to decay, heating or cooling photons passing through density crests or troughs. In a flat universe, the linear ISW effect is a direct signal of dark energy.

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10.1086/591670