The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space
Abstract
We investigate the anisotropic clustering of the Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 sample, which consists of 1198 006 galaxies in the redshift range 0.2 < z < 0.75 and a sky coverage of 10 252 deg2. We analyse this data set in Fourier space, using the power-spectrum multipoles to measure redshift-space distortions simultaneously with the Alcock–Paczynski effect and the baryon acoustic oscillation scale. We include the power-spectrum monopole, quadrupole and hexadecapole in our analysis and compare our measurements with a perturbation-theory-based model, while properly accounting for the survey window function. To evaluate the reliability of our analysis pipeline, we participate in a mock challenge, which results in systematic uncertainties significantly smaller than the statistical uncertainties. While the high-redshift constraint on fσ8 at zeff = 0.61 indicates a small (~1.4σ) deviation from the prediction of the Planck ΛCDM (Λ cold dark matter) model, the low-redshift constraint is in good agreement with Planck ΛCDM. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. Lastly, the measurements and likelihoods presented here are combined with others in Alam et al. to produce the final cosmological constraints from BOSS.
- Authors:
-
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- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology & Gravitation; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Ohio Univ., Athens, OH (United States). Dept. of Physics and Astronomy
- Max Planck Inst. fur Astrophysik, Garching bei Munchen (Germany); Univ. of Tokyo (Japan). Inst. for Advanced Study, Kavli Inst. for the Physics and Mathematics of the Universe (WPI)
- Leibniz Inst. fur Astrophysik Potsdam (AIP), Potsdam (Germany); Univ. Autonoma de Madrid (Spain). Dept. de Fisica Teorica
- Univ. de Barcelona (Spain). Inst. de Ciencies del Cosmos (ICCUB)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Sorbonne Univ., Paris (France). Inst. Lagrange de Paris; Univ. Pierre et Marie Curie, Paris (France). Lab. de Physique Nuclaire et de Hautes Energies
- Ludwig Maximilian Univ., Munich (Germany). Univ. Sternwarte Munchen; Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
- Univ. of California, Berkeley, CA (United States). Dept. of Astronomy
- Leibniz Inst. fur Astrophysik Potsdam (AIP), Potsdam (Germany)
- Univ. of California, Berkeley, CA (United States). Dept. of Physics
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology & Gravitation
- Pennsylvania State Univ., University Park, PA (United States). Inst. for Gravitation and the Cosmos
- Inst. de Astrofisica de Andalucia (CSIC), Granada (Spain); Campus of International Excellence UAM+CSIC, Madrid (Spain); Univ. Autonoma de Madrid (Spain). Dept. de Fisica Teorica
- Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
- Univ. Autonoma de Madrid (Spain). Dept. de Fisica Teorica; Campus of International Excellence UAM+CSIC, Madrid (Spain)
- Sorbonne Univ., Paris (France). Inst. Lagrange de Paris; Univ. of Portsmouth (United Kingdom). Inst. of Cosmology & Gravitation
- Univ. of Edinburgh, Scotland (United Kingdom). The Royal Observatory, Inst. for Astronomy
- Pennsylvania State Univ., University Park, PA (United States). Dept. of Astronomy and Astrophysics; Pennsylvania State Univ., University Park, PA (United States). Inst. for Gravitation and the Cosmos
- New York Univ. (NYU), NY (United States). Dept. of Physics, Center for Cosmology and Particle Physics
- Univ. of St. Andrews, Scotland (United Kingdom). School of Phsyics and Astronomy
- Univ. Nacional Autonoma de Mexico (UNAM), Mexico City (Mexico). Inst. de Fisica
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
- OSTI Identifier:
- 1526477
- Grant/Contract Number:
- AC02-05CH11231; SC0014329; CSD2009-00064; SEV-2012-0249; AYA2014-60641-C2-1-P
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 466; Journal Issue: 2; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 97 MATHEMATICS AND COMPUTING
Citation Formats
Beutler, Florian, Seo, Hee-Jong, Saito, Shun, Chuang, Chia-Hsun, Cuesta, Antonio J., Eisenstein, Daniel J., Gil-Marín, Héctor, Grieb, Jan Niklas, Hand, Nick, Kitaura, Francisco-Shu, Modi, Chirag, Nichol, Robert C., Olmstead, Matthew D., Percival, Will J., Prada, Francisco, Sánchez, Ariel G., Rodriguez-Torres, Sergio, Ross, Ashley J., Ross, Nicholas P., Schneider, Donald P., Tinker, Jeremy, Tojeiro, Rita, and Vargas-Magaña, Mariana. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space. United States: N. p., 2016.
Web. doi:10.1093/mnras/stw3298.
Beutler, Florian, Seo, Hee-Jong, Saito, Shun, Chuang, Chia-Hsun, Cuesta, Antonio J., Eisenstein, Daniel J., Gil-Marín, Héctor, Grieb, Jan Niklas, Hand, Nick, Kitaura, Francisco-Shu, Modi, Chirag, Nichol, Robert C., Olmstead, Matthew D., Percival, Will J., Prada, Francisco, Sánchez, Ariel G., Rodriguez-Torres, Sergio, Ross, Ashley J., Ross, Nicholas P., Schneider, Donald P., Tinker, Jeremy, Tojeiro, Rita, & Vargas-Magaña, Mariana. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space. United States. https://doi.org/10.1093/mnras/stw3298
Beutler, Florian, Seo, Hee-Jong, Saito, Shun, Chuang, Chia-Hsun, Cuesta, Antonio J., Eisenstein, Daniel J., Gil-Marín, Héctor, Grieb, Jan Niklas, Hand, Nick, Kitaura, Francisco-Shu, Modi, Chirag, Nichol, Robert C., Olmstead, Matthew D., Percival, Will J., Prada, Francisco, Sánchez, Ariel G., Rodriguez-Torres, Sergio, Ross, Ashley J., Ross, Nicholas P., Schneider, Donald P., Tinker, Jeremy, Tojeiro, Rita, and Vargas-Magaña, Mariana. Sat .
"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space". United States. https://doi.org/10.1093/mnras/stw3298. https://www.osti.gov/servlets/purl/1526477.
@article{osti_1526477,
title = {The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space},
author = {Beutler, Florian and Seo, Hee-Jong and Saito, Shun and Chuang, Chia-Hsun and Cuesta, Antonio J. and Eisenstein, Daniel J. and Gil-Marín, Héctor and Grieb, Jan Niklas and Hand, Nick and Kitaura, Francisco-Shu and Modi, Chirag and Nichol, Robert C. and Olmstead, Matthew D. and Percival, Will J. and Prada, Francisco and Sánchez, Ariel G. and Rodriguez-Torres, Sergio and Ross, Ashley J. and Ross, Nicholas P. and Schneider, Donald P. and Tinker, Jeremy and Tojeiro, Rita and Vargas-Magaña, Mariana},
abstractNote = {We investigate the anisotropic clustering of the Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 sample, which consists of 1198 006 galaxies in the redshift range 0.2 < z < 0.75 and a sky coverage of 10 252 deg2. We analyse this data set in Fourier space, using the power-spectrum multipoles to measure redshift-space distortions simultaneously with the Alcock–Paczynski effect and the baryon acoustic oscillation scale. We include the power-spectrum monopole, quadrupole and hexadecapole in our analysis and compare our measurements with a perturbation-theory-based model, while properly accounting for the survey window function. To evaluate the reliability of our analysis pipeline, we participate in a mock challenge, which results in systematic uncertainties significantly smaller than the statistical uncertainties. While the high-redshift constraint on fσ8 at zeff = 0.61 indicates a small (~1.4σ) deviation from the prediction of the Planck ΛCDM (Λ cold dark matter) model, the low-redshift constraint is in good agreement with Planck ΛCDM. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. Lastly, 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/stw3298},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 466,
place = {United States},
year = {Sat Dec 17 00:00:00 EST 2016},
month = {Sat Dec 17 00:00:00 EST 2016}
}
Web of Science
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