The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
Chris Blake, Ixandra Achitouv, Angela Burden, Yann Rasera

TL;DR
This study investigates how galaxy environment affects the baryon acoustic peak in the BOSS CMASS sample, finding the distance scale is environment-independent but the peak shape varies, and optimizing weighting improves measurement precision.
Contribution
It demonstrates that environmental weighting enhances BAO measurement precision and confirms the peak's shape dependence on local density, with implications for galaxy clustering analyses.
Findings
Distance scale is environment-independent.
Peak shape varies with environment.
Weighted analysis improves BAO fit precision.
Abstract
The environmental dependence of galaxy clustering encodes information about the physical processes governing the growth of cosmic structure. We analyze the baryon acoustic peak as a function of environment in the galaxy correlation function of the Baryon Oscillation Spectroscopic Survey CMASS sample. Dividing the sample into three subsets by smoothed local overdensity, we detect acoustic peaks in the six separate auto-correlation and cross-correlation functions of the sub-samples. Fitting models to these correlation functions, calibrated by mock galaxy and dark matter catalogues, we find that the inferred distance scale is independent of environment, and consistent with the result of analyzing the combined sample. The shape of the baryon acoustic feature, and the accuracy of density-field reconstruction in the Zeldovich approximation, varies with environment. By up-weighting underdense…
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