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- W2049486583 endingPage "2086" @default.
- W2049486583 startingPage "2078" @default.
- W2049486583 abstract "We measure the matter probability distribution function (PDF) via counts in cells in a volume limited subsample of the Sloan Digital Sky Survey Luminous Red Galaxy Catalog on scales from $30 h^{-1}$Mpc to $150 h^{-1}$Mpc and estimate the linear Integrated Sachs--Wolfe effect produced by supervoids and superclusters in the tail of the PDF. We characterize the PDF by the variance, $S_3$, and $S_4$, and study in simulations the systematic effects due to finite volume, survey shape and redshift distortion. We compare our measurement to the prediction of $Lambda$CDM with linear bias and find a good agreement. We use the moments to approximate the tail of the PDF with analytic functions. A simple Gaussian model for the superstructures appears to be consistent with the claim by Granett et al. that density fluctuations on $100 h^{-1}$Mpc scales produce hot and cold spots with $Delta T approx 10mu K$ on the cosmic microwave background." @default.
- W2049486583 created "2016-06-24" @default.
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- W2049486583 date "2010-12-03" @default.
- W2049486583 modified "2023-09-23" @default.
- W2049486583 title "COSMOLOGICAL DENSITY FLUCTUATIONS ON 100 Mpc SCALES AND THEIR ISW EFFECT" @default.
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- W2049486583 doi "https://doi.org/10.1088/0004-637x/725/2/2078" @default.
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