Galaxy bias and its effects on the baryon acoustic oscillation measurements

Kushal T. Mehta, Hee Jong Seo, Jonathan Eckel, Daniel J. Eisenstein, Marc Metchnik, Philip Pinto, Xiaoying Xu

Research output: Contribution to journalArticle

65 Scopus citations

Abstract

The baryon acoustic oscillation (BAO) feature in the clustering of matter in the universe serves as a robust standard ruler and hence can be used to map the expansion history of the universe. We use high force resolution simulations to analyze the effects of galaxy bias on the measurements of the BAO signal. We apply a variety of Halo Occupation Distributions (HODs) and produce biased mass tracers to mimic different galaxy populations. We investigate whether galaxy bias changes the nonlinear shifts on the acoustic scale relative to the underlying dark matter distribution presented by Seo etal. For the less biased HOD models (b < 3), we do not detect any shift in the acoustic scale relative to the no-bias case, typically 0.10% ± 0.10%. However, the most biased HOD models (b > 3) show a shift at moderate significance (0.79% ± 0.31% for the most extreme case). We test the one-step reconstruction technique introduced by Eisenstein etal. in the case of realistic galaxy bias and shot noise. The reconstruction scheme increases the correlation between the initial and final (z = 1) density fields, achieving an equivalent level of correlation at nearly twice the wavenumber after reconstruction. Reconstruction reduces the shifts and errors on the shifts. We find that after reconstruction the shifts from the galaxy cases and the dark matter case are consistent with each other and with no shift. The 1σ systematic errors on the distance measurements inferred from our BAO measurements with various HODs after reconstruction are about 0.07%-0.15%.

Original languageEnglish (US)
Article number94
JournalAstrophysical Journal
Volume734
Issue number2
DOIs
StatePublished - Jun 10 2011

Keywords

  • cosmological parameters
  • cosmology: theory
  • dark energy
  • dark matter
  • distance scale
  • large-scale structure of universe

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Mehta, K. T., Seo, H. J., Eckel, J., Eisenstein, D. J., Metchnik, M., Pinto, P., & Xu, X. (2011). Galaxy bias and its effects on the baryon acoustic oscillation measurements. Astrophysical Journal, 734(2), [94]. https://doi.org/10.1088/0004-637X/734/2/94