Correlation of CMB with large-scale structure. II. Weak lensing

Christopher M. Hirata, Shirley Ho, Nikhil Padmanabhan, Uroš Seljak, Neta A. Bahcall

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156 Scopus citations

Abstract

We investigate the correlation of gravitational lensing of the cosmic microwave background (CMB) with several tracers of large-scale structure, including luminous red galaxies (LRGs), quasars, and radio sources. The lensing field is reconstructed based on the CMB maps from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite; the LRGs and quasars are observed by the Sloan Digital Sky Survey (SDSS); and the radio sources are observed in the NRAO VLA Sky Survey (NVSS). Combining all three large-scale structure samples, we find evidence for a positive cross correlation at the 2.5σ level (1.8σ for the SDSS samples and 2.1σ for NVSS); the cross correlation amplitude is 1.06±0.42 times that expected for the WMAP cosmological parameters. Our analysis extends other recent analyses in that we carefully determine bias-weighted redshift distribution of the sources, which is needed for a meaningful cosmological interpretation of the detected signal. We investigate contamination of the signal by galactic emission, extragalactic radio and infrared sources, thermal and kinetic Sunyaev-Zel'dovich effects, and the Rees-Sciama effect, and find all of them to be negligible.

Original languageEnglish (US)
Article number043520
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume78
Issue number4
DOIs
StatePublished - Aug 13 2008

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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