An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
Benjamin R. Granett, Mark C. Neyrinck, and Istv\'an Szapudi (IfA,, Hawaii)

TL;DR
This paper detects the late-time Integrated Sachs-Wolfe effect by measuring temperature deviations in the microwave background associated with super-structures, providing evidence for dark energy in a flat universe.
Contribution
It presents the first direct observational evidence linking super-structures to the ISW effect using SDSS data, supporting the existence of dark energy.
Findings
Mean temperature deviation of 9.6 microK with 4 sigma significance
Visual imprint of super-structures on the microwave background
Detection consistent with predictions of dark energy effects
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 microK, i.e. above 4 sigma. 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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