Clustering of luminous red galaxies - IV. Baryon acoustic peak in the line-of-sight direction and a direct measurement of H ( z )

Institute of Space Sciences · Columbia University

Indexed inarxivcrossrefdoaj

Abstract

We study the clustering of LRG galaxies in the latest spectroscopic SDSS data releases, DR6 and DR7, which sample over 1 Gpc^3/h^3 to z=0.47. The 2-point correlation function $\xisp$ is estimated as a function of perpendicular $\sigma$ and line-of-sight $\pi$ (radial) directions. We find a significant detection of a peak at $r\simeq 110$Mpc/h, which shows as a circular ring in the $\sigma-\pi$ plane. There is also significant evidence for a peak along the radial direction whose shape is consistent with its originating from the recombination-epoch baryon acoustic oscillations (BAO). A $\xisp$ model with no radial BAO peak is disfavored at $3.2\sigma$, whereas a model with no magnification bias is disfavored at…

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Topics & keywords

Keywords
  • Physics
  • Astrophysics
  • Redshift
  • Galaxy
  • Baryon acoustic oscillations
  • Line-of-sight
  • Correlation function (quantum field theory)
  • Baryon
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