Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry

TL;DR

This paper introduces a cross-correlation method between sparse spectroscopic and dense photometric samples to improve BAO measurements, demonstrated with SDSS data, showing promising results for future cosmological distance scale studies.

Contribution

The paper develops and applies a novel formalism for BAO analysis using cross-correlation, reducing shot noise and enhancing measurement precision compared to traditional auto-correlation methods.

Findings

Detected BAO peak at 2.8sigma significance in cross-correlation

Measured angular diameter distance at z=0.64 as 2418 +/- 73 Mpc

Demonstrated potential for improved BAO measurements with future data

Abstract

We develop a formalism for measuring the cosmological distance scale from baryon acoustic oscillations (BAO) using the cross-correlation of a sparse redshift survey with a denser photometric sample. This reduces the shot noise that would otherwise affect the auto-correlation of the sparse spectroscopic map. As a proof of principle, we make the first on-sky application of this method to a sparse sample defined as the z>0.6 tail of the Sloan Digital Sky Survey's (SDSS) BOSS/CMASS sample of galaxies and a dense photometric sample from SDSS DR9. We find a 2.8sigma preference for the BAO peak in the cross-correlation at an effective z=0.64, from which we measure the angular diameter distance D_M(z=0.64) = (2418 +/- 73 Mpc) (r_s/r_{s,fid}). Accordingly, we expect that using this method to combine sparse spectroscopy with the deep, high quality imaging that is just now becoming available will enable higher precision BAO measurements than possible with the spectroscopy alone.