Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
H.J. Tian, Mark C. Neyrinck, Tam\'as Budav\'ari, Alexander S. Szalay, (JHU)

TL;DR
This paper investigates how redshift-space distortions enhance the visibility of baryon acoustic oscillations along the line of sight, using simulations and SDSS data, revealing a sharper BAO feature with increased significance.
Contribution
It demonstrates that redshift-space distortions can sharpen BAO features along the line of sight, and provides observational evidence from SDSS data supporting this effect.
Findings
Redshift-space distortions make BAO features sharper along the line of sight.
A localized BAO bump was detected at approximately 110 Mpc/h with 4 sigma significance.
The probability of such a signal arising from a non-BAO power spectrum is about 0.2%.
Abstract
We show that redshift-space distortions of galaxy correlations have a strong effect on correlation functions with distinct, localized features, like the signature of the baryon acoustic oscillations (BAO). Near the line of sight, the features become sharper as a result of redshift-space distortions. We demonstrate this effect by measuring the correlation function in Gaussian simulations and the Millennium Simulation. We also analyze the SDSS DR7 main-galaxy sample (MGS), splitting the sample into slices 2.5 degrees on the sky in various rotations. Measuring 2D correlation functions in each slice, we do see a sharp bump along the line of sight. Using Mexican-hat wavelets, we localize it to (110 +/- 10) Mpc/h. Averaging only along the line of sight, we estimate its significance at a particular wavelet scale and location at 2.2 sigma. In a flat angular weighting in the (pi,r_p) coordinate…
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