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 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 < z < 0.75. These galaxy samples are categorized in three redshift bins. Using CLPT-GSRSD in our analysis of the combined sample of the three redshift bins, we report measurements of fσ8 for the three redshift bins. We find fσ8 = 0.430 ± 0.054 at zeff = 0.38, fσ8 = 0.452 ± 0.057 at zeff = 0.51 and fσ8 = 0.457 ± 0.052 at zeff = 0.61. Our results are consistent with the predictions of Planck Λ cold dark matter-general relativity. Our constraints on the growth rates of structure in the Universe at different redshifts serve as a useful probe, which can help distinguish between a model of the Universe based on dark energy and models based on modified theories of gravity. This paper is part of a set that analyses the finalmore »
- Authors:
-
- Carnegie Mellon Univ., Pittsburgh, PA (United States)
- Carnegie Mellon Univ., Pittsburgh, PA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Princeton Univ., NJ (United States)
- Univ. of Portsmouth (United Kingdom)
- Univ. of Utah, Salt Lake City, UT (United States)
- Univ. Autonoma de Madrid (Spain); Leibniz Inst. for Astrophyics Potsdam (AIP) Germany)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Ludwig Maximilian Univ., Munich (Germany); Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States); Leibniz Inst. for Astrophyics Potsdam (AIP) Germany)
- King's College, Wilkes Barre, PA (United States)
- Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
- Ohio Univ., Athens, OH (United States)
- New York Univ. (NYU), NY (United States)
- Univ. of St. Andrews, Scotland (United Kingdom)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1530267
- Alternate Identifier(s):
- OSTI ID: 1594737
- Grant/Contract Number:
- AC02-05CH11231; SC0017860
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 469; Journal Issue: 2; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
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., and Tojeiro, Rita. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions. United States: N. p., 2017.
Web. doi:10.1093/mnras/stx883.
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. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions. United States. https://doi.org/10.1093/mnras/stx883
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., and Tojeiro, Rita. Tue .
"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions". United States. https://doi.org/10.1093/mnras/stx883. https://www.osti.gov/servlets/purl/1530267.
@article{osti_1530267,
title = {The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions},
author = {Satpathy, Siddharth and Alam, Shadab and Ho, Shirley and White, Martin and Bahcall, Neta A. and Beutler, Florian and Brownstein, Joel R. and Chuang, Chia-Hsun and Eisenstein, Daniel J. and Grieb, Jan Niklas and Kitaura, Francisco and Olmstead, Matthew D. and Percival, Will J. and Salazar-Albornoz, Salvador and Sánchez, Ariel G. and Seo, Hee-Jong and Thomas, Daniel and Tinker, Jeremy L. and Tojeiro, Rita},
abstractNote = {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 < z < 0.75. These galaxy samples are categorized in three redshift bins. Using CLPT-GSRSD in our analysis of the combined sample of the three redshift bins, we report measurements of fσ8 for the three redshift bins. We find fσ8 = 0.430 ± 0.054 at zeff = 0.38, fσ8 = 0.452 ± 0.057 at zeff = 0.51 and fσ8 = 0.457 ± 0.052 at zeff = 0.61. Our results are consistent with the predictions of Planck Λ cold dark matter-general relativity. Our constraints on the growth rates of structure in the Universe at different redshifts serve as a useful probe, which can help distinguish between a model of the Universe based on dark energy and models based on modified theories of gravity. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are combined with others in Alam et al., to produce the final cosmological constraints from BOSS.},
doi = {10.1093/mnras/stx883},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 469,
place = {United States},
year = {Tue Apr 11 00:00:00 EDT 2017},
month = {Tue Apr 11 00:00:00 EDT 2017}
}
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