The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions

Abstract We present a measurement of the linear growth rate of structure, f, from the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using convolution Lagrangian perturbation theory (CLPT) with Gaussian streaming redshift space distortio...

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Published in:Monthly notices of the Royal Astronomical Society 2017-08, Vol.469 (2), p.1369-1382
Main Authors: Satpathy, Siddharth, Alam, Shadab, Ho, Shirley, White, Martin, Bahcall, Neta A., Beutler, Florian, Brownstein, Joel R., Chuang, Chia-Hsun, Eisenstein, Daniel J., Grieb, Jan Niklas, Kitaura, Francisco, Olmstead, Matthew D., Percival, Will J., Salazar-Albornoz, Salvador, Sánchez, Ariel G., Seo, Hee-Jong, Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita
Format: Article
Language:English
Subjects:
ASTRONOMY AND ASTROPHYSICS
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Summary:Abstract We present a measurement of the linear growth rate of structure, f, from the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using convolution Lagrangian perturbation theory (CLPT) with Gaussian streaming redshift space distortions (GSRSD) to model the two-point statistics of BOSS galaxies in DR12. The BOSS-DR12 data set includes 1198 006 massive galaxies spread over the redshift range 0.2 
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stx883