The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
Abstract
In this work, we perform a tomographic baryon acoustic oscillations (BAO) analysis using the monopole, quadrupole and hexadecapole of the redshift-space galaxy power spectrum measured from the pre-reconstructed combined galaxy sample of the completed Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey (BOSS) Data Release12 covering the redshift range of 0.20 < z < 0.75. By allowing for overlap between neighbouring redshift slices, we successfully obtained the isotropic and anisotropic BAO distance measurements within nine redshift slices to a precision of 1.5–3.4 percent for DV/rd, 1.8–4.2 percent for DA/rd and 3.7–7.5 percent for H rd, depending on effective redshifts. We provide our BAO measurement of DA/rd and H rd with the full covariance matrix, which can be used for cosmological implications. Our measurements are consistent with those presented in Alam et al., in which the BAO distances are measured at three effective redshifts. We constrain dark energy parameters using our measurements and find an improvement of the Figure-of-Merit of dark energy in general due to the temporal BAO information resolved. Finally, this paper is a part of a set that analyses the final galaxy clustering data set from BOSS.
- Authors:
-
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- Chinese Academy of Sciences (CAS), Beijing (China). National Astronomy Observatories; Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation
- Univ. of Tokyo (Japan). Kavli Inst. for the Physics and Mathematics of the Universe (IPMU); Max Planck Inst. fur Astrophysik, Garching (Germany)
- Chinese Academy of Sciences (CAS), Beijing (China). National Astronomy Observatories
- The Ohio State Univ., Columbus, OH (United States). Center for Cosmology and AstroParticle Physics; Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Ludwig Maximilian Univ., Munich (Germany) Univ. Sternwarte Munchen; Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
- Leibniz Inst. fur Astrphysik Potsdam (AIP), Potsdam (Germany); Univ. Autonoma de Madrid (Spain). Dept. de Fisica Teorica
- Leibniz Inst. fur Astrophysik Potsdam (AIP), Potsdam (Germany)
- Campus of International Excellence, Madrid (Spain); Univ. Autonoma de Madrid (Spain). Dept. de Fisica Teorica
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation
- Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy
- Univ. of Barcelona (Spain). Inst. de Ciencies del Cosmos (ICCUB)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation; Sorbonne Univ., Paris (France). Inst. Lagrange de Paris (ILP); Univ. Pierre et Marie Curie, Paris (France). Lab. de Physique Nucleaire et de Huates Energies
- Ecole Polytechnique Federale Lausanne (Switzlerland). Lab. d'Astrophysique
- King's College, Wilkes Barre, PA (United States). Dept. of Chemistry and Physics
- Univ. Autonoma de Madrid (Spain). Dept. de Fisica Teorica
- Sejong Univ., Seoul (Korea, Republic of). Dept. of Astronomy and Space Science
- Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany); Ludwig Maximilian Univ., Munich (Germany)
- Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
- New York Univ. (NYU), NY (United States). Center for Cosmology and Particle Physics, Dept. of Physics
- Univ. of St. Andrews, Scotland (United Kingdom). School of Physics and Astronomy
- The Ohio State Univ., Columbus, OH (United States). Dept. of Astronomy; The Ohio State Univ., Columbus, OH (United States). Center for Cosmology and AstroParticle Physics
- Yale Univ., New Haven, CT (United States). Dept. of Physics
- 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)
- OSTI Identifier:
- 1526320
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 466; Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; galaxies: distances and redshifts; cosmological parameters; cosmology: observations; dark energy; distance scale; large-scale structure of Universe
Citation Formats
Zhao, Gong-Bo, Wang, Yuting, Saito, Shun, Wang, Dandan, Ross, Ashley J., Beutler, Florian, Grieb, Jan Niklas, Chuang, Chia-Hsun, Kitaura, Francisco-Shu, Rodriguez-Torres, Sergio, Percival, Will J., Brownstein, Joel R., Cuesta, Antonio J., Eisenstein, Daniel J., Gil-Marín, Héctor, Kneib, Jean-Paul, Nichol, Robert C., Olmstead, Matthew D., Prada, Francisco, Rossi, Graziano, Salazar-Albornoz, Salvador, Samushia, Lado, Sánchez, Ariel G., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Weinberg, David H., and Zhu, Fangzhou. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space. United States: N. p., 2016.
Web. doi:10.1093/mnras/stw3199.
Zhao, Gong-Bo, Wang, Yuting, Saito, Shun, Wang, Dandan, Ross, Ashley J., Beutler, Florian, Grieb, Jan Niklas, Chuang, Chia-Hsun, Kitaura, Francisco-Shu, Rodriguez-Torres, Sergio, Percival, Will J., Brownstein, Joel R., Cuesta, Antonio J., Eisenstein, Daniel J., Gil-Marín, Héctor, Kneib, Jean-Paul, Nichol, Robert C., Olmstead, Matthew D., Prada, Francisco, Rossi, Graziano, Salazar-Albornoz, Salvador, Samushia, Lado, Sánchez, Ariel G., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Weinberg, David H., & Zhu, Fangzhou. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space. United States. https://doi.org/10.1093/mnras/stw3199
Zhao, Gong-Bo, Wang, Yuting, Saito, Shun, Wang, Dandan, Ross, Ashley J., Beutler, Florian, Grieb, Jan Niklas, Chuang, Chia-Hsun, Kitaura, Francisco-Shu, Rodriguez-Torres, Sergio, Percival, Will J., Brownstein, Joel R., Cuesta, Antonio J., Eisenstein, Daniel J., Gil-Marín, Héctor, Kneib, Jean-Paul, Nichol, Robert C., Olmstead, Matthew D., Prada, Francisco, Rossi, Graziano, Salazar-Albornoz, Salvador, Samushia, Lado, Sánchez, Ariel G., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Weinberg, David H., and Zhu, Fangzhou. Sun .
"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space". United States. https://doi.org/10.1093/mnras/stw3199. https://www.osti.gov/servlets/purl/1526320.
@article{osti_1526320,
title = {The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space},
author = {Zhao, Gong-Bo and Wang, Yuting and Saito, Shun and Wang, Dandan and Ross, Ashley J. and Beutler, Florian and Grieb, Jan Niklas and Chuang, Chia-Hsun and Kitaura, Francisco-Shu and Rodriguez-Torres, Sergio and Percival, Will J. and Brownstein, Joel R. and Cuesta, Antonio J. and Eisenstein, Daniel J. and Gil-Marín, Héctor and Kneib, Jean-Paul and Nichol, Robert C. and Olmstead, Matthew D. and Prada, Francisco and Rossi, Graziano and Salazar-Albornoz, Salvador and Samushia, Lado and Sánchez, Ariel G. and Thomas, Daniel and Tinker, Jeremy L. and Tojeiro, Rita and Weinberg, David H. and Zhu, Fangzhou},
abstractNote = {In this work, we perform a tomographic baryon acoustic oscillations (BAO) analysis using the monopole, quadrupole and hexadecapole of the redshift-space galaxy power spectrum measured from the pre-reconstructed combined galaxy sample of the completed Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey (BOSS) Data Release12 covering the redshift range of 0.20 < z < 0.75. By allowing for overlap between neighbouring redshift slices, we successfully obtained the isotropic and anisotropic BAO distance measurements within nine redshift slices to a precision of 1.5–3.4 percent for DV/rd, 1.8–4.2 percent for DA/rd and 3.7–7.5 percent for H rd, depending on effective redshifts. We provide our BAO measurement of DA/rd and H rd with the full covariance matrix, which can be used for cosmological implications. Our measurements are consistent with those presented in Alam et al., in which the BAO distances are measured at three effective redshifts. We constrain dark energy parameters using our measurements and find an improvement of the Figure-of-Merit of dark energy in general due to the temporal BAO information resolved. Finally, this paper is a part of a set that analyses the final galaxy clustering data set from BOSS.},
doi = {10.1093/mnras/stw3199},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 466,
place = {United States},
year = {Sun Dec 11 00:00:00 EST 2016},
month = {Sun Dec 11 00:00:00 EST 2016}
}
Web of Science
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