The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
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We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III.Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg 2 and volume of 18.7 Gpc 3 , divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61.We measure the angular diameter distance D M and Hubble parameter H from the baryon acoustic oscillation (BAO) method, in combination with a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature.Using the anisotropic clustering of the Hubble Fellow.
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Alam et al. (2017a) note that the current growth measurements of f sigma8 reaffirm the validity of GR.
“The authors note that the current growth measurements of reaffirm the validity of GR.”
From Testing general relativity in cosmology (2019) · cites this paper as Alam et al. (2017a)
Alam et al. (2017a) found very little changes in these values when allowing the equation of state w and the spatial curvature parameter to vary.
“They also found very little changes in these values when they allow for the equation of state w and the spatial curvature parameter to vary.”
From Testing general relativity in cosmology (2019) · cites this paper as Alam et al. (2017a)
Alam et al. (2017a) combined RSD and BAO with Planck-2015 and, for a LCDM background model and redshift-independent rescaling, found a growth amplitude value consistent with GR.
“For a CDM background model and a redshift independent rescaling, they find , so a growth amplitude value that is consistent with GR.”
From Testing general relativity in cosmology (2019) · cites this paper as Alam et al. (2017a)
Alam et al. (2017a), when allowing redshift-dependent variation, found a 1.5-sigma deviation from a zero GR-value, which they considered not statistically significant and concluded their results are consistent with GR.
“When they allow for a redshift-dependent variation, they find and . This is a 1.5- deviation from a zero GR-value so they considered this as not statistically significant and concluded that their results are consistent with GR.”
From Testing general relativity in cosmology (2019) · cites this paper as Alam et al. (2017a)
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Self-citationTeleparallel gravity: from theory to cosmology
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Self-citationCosmological parameters from the BOSS galaxy power spectrum
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Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument
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Self-citationMeasurement of baryon acoustic oscillation correlations atz = 2.3 with SDSS DR12 Lyα-Forests
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Self-citationNonminimal dark sector physics and cosmological tensions
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Oscillating scalar fields and the Hubble tension: A resolution with novel signatures
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Self-citationDark energy two decades after: observables, probes, consistency tests
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Self-citationUnveiling the Universe with emerging cosmological probes
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Self-citationFirst evidence that non-metricity f(Q) gravity could challenge ΛCDM
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Self-citationnbodykit: An Open-source, Massively Parallel Toolkit for Large-scale Structure
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Self-citationDoes the Hubble constant tension call for new physics?
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Self-citationDark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing
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Self-citationDark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data
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Baryon acoustic oscillations at z = 2.34 from the correlations of Lyα absorption in eBOSS DR14
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Self-citationBaryon acoustic oscillations from the cross-correlation of Ly α absorption and quasars in eBOSS DR14
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Self-citationConstraints on the Cosmic Expansion History from GWTC–3
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Self-citationUnion through UNITY: Cosmology with 2000 SNe Using a Unified Bayesian Framework
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Acoustic dark energy: Potential conversion of the Hubble tension
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- Authors
- Alam, S., Ata, M., Bailey, S., Beutler, F., Bizyaev, D., Blazek, J. A., Bolton, A. S., Brownstein, J. R., Burden, A., Chuang, C.-H., Comparat, J., Cuesta, A. J., Dawson, K. S., Eisenstein, D. J., Escoffier, S., Gil-Marín, H., Grieb, J. N., Hand, N., Ho, S., Kinemuchi, K., Kirkby, D., Kitaura, F., Malanushenko, E., Malanushenko, V., Maraston, C., McBride, C. K., Nichol, R. C., Olmstead, M. D., Oravetz, D., Padmanabhan, N., Palanque-Delabrouille, N., Pan, K., Pellejero-Ibanez, M., Percival, W. J., Petitjean, P., Prada, F., Price-Whelan, A. M., Reid, B. A., Rodríguez-Torres, S. A., Roe, N. A., Ross, A. J., Ross, N. P., Rossi, G., Rubiño-Martín, J. A., Saito, S., Salazar-Albornoz, S., Samushia, L., Sánchez, A. G., Satpathy, S., Schlegel, D. J., Schneider, D. P., Scóccola, C. G., Seo, H.-J., Sheldon, E. S., Simmons, A., Slosar, A., Strauss, M. A., Swanson, M. E. C., Thomas, D., Tinker, J. L., Tojeiro, R., Magaña, M. V., Vazquez, J. A., Verde, L., Wake, D. A., Wang, Y., Weinberg, D. H., White, M., Wood-Vasey, W. M., Yèche, C., Zehavi, I., Zhai, Z., & Zhao, G.-B.
- Affiliations
- Carnegie Mellon University (US)
- Leibniz Institute for Astrophysics Potsdam (DE)
- Lawrence Berkeley National Laboratory (US)
- New Mexico State University (US)
- The Ohio State University (US)
- University of Utah (US)
- Yale University (US)
- Instituto de Física Teórica (ES)
- Institut de Ciències del Cosmos (ES)
- Center for Astrophysics Harvard & Smithsonian (US)
- Centre National de la Recherche Scientifique (FR)
- Sorbonne Université (FR)
- Max Planck Institute for Extraterrestrial Physics (DE)
- University of California, Berkeley (US)
- University of California, Irvine (US)
- University of Portsmouth (GB)
- King's College - Pennsylvania (US)
- Consejo Superior de Investigaciones Científicas (ES)
- Princeton University (US)
- Centre de physique des particules de Marseille (FR)
- Sejong University (KR)
- Kavli Institute for the Physics and Mathematics of the Universe (JP)
- Kansas State University (US)
- Pennsylvania State University (US)
- Consejo Nacional de Investigaciones Científicas y Técnicas (AR)
- Brookhaven National Laboratory (US)
- University of St Andrews (GB)
- Institució Catalana de Recerca i Estudis Avançats (ES)
- University of Wisconsin–Madison (US)
- Chinese Academy of Sciences (CN)
- Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR)
- Corresponding author
- Reid, Beth A.
- Tinker, Jeremy L.
- ORCID
- Alam, Shadab
- Ata, Metin
- Bailey, Stephen
- Beutler, Florian
- Bizyaev, Dmitry
- Blazek, Jonathan A.
- Bolton, Adam S.
- Brownstein, Joel R.
- Burden, Angela
- Chuang, Chia-Hsun
- Comparat, Johan
- Cuesta, Antonio J.
- Dawson, Kyle S.
- Eisenstein, Daniel J.
- Escoffier, Stephanie
- Gil-Marín, Héctor
- Grieb, Jan Niklas
- Hand, Nick
- Ho, Shirley
- Kinemuchi, Karen
- Kirkby, David
- Kitaura, Francisco
- Maraston, Claudia
- Nichol, Robert C.
- Padmanabhan, Nikhil
- Pan, Kaike
- Percival, Will J.
- Petitjean, Patrick
- Prada, Francisco
- Price-Whelan, Adrian M.
- Reid, Beth A.
- Ross, Ashley J.
- Ross, Nicholas P.
- Saito, Shun
- Samushia, Lado
- Sánchez, Ariel G.
- Satpathy, Siddharth
- Schlegel, David J.
- Schneider, Donald P.
- Scóccola, Claudia G.
- Seo, Hee-Jong
- Sheldon, Erin S.
- Simmons, Audrey
- Slosar, Anže
- Strauss, Michael A.
- Swanson, Molly E. C.
- Thomas, Daniel
- Tinker, Jeremy L.
- Tojeiro, Rita
- Vazquez, Jose Alberto
- Verde, Licia
- Wake, David A.
- Wang, Yuting
- Weinberg, David H.
- White, Martin
- Yèche, Christophe
- Zehavi, Idit
- Zhai, Zhongxu
- Zhao, Gong-Bo
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2017-03-28
- Volume
- 470
- Issue
- 3
- Pages
- 2617-2652
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2501864044
- Cited by
- 3,056
- References
- 221
- Citations by year
- 2026: 203 · 2025: 375 · 2024: 411 · 2023: 353 · 2022: 353 · 2021: 375 · 2020: 380 · 2019: 291 · 2018: 200 · 2017: 100 · 2016: 14 · 2015: 1
- FWCI
- 142.23
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- RECERCAT (Consorci de Serveis Universitaris de Catalunya) (publishedVersion)
- Open Research Online - ORO (The Open University) (acceptedVersion)
- DIGITAL.CSIC (Spanish National Research Council (CSIC)) (acceptedVersion)
- arXiv (Cornell University) (submittedVersion)
- St Andrews Research Repository (St Andrews Research Repository) (submittedVersion)
- LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) (submittedVersion, cc-by-nc-sa)
- eScholarship (California Digital Library) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- HAL (submittedVersion, other-oa)
- Americanae (AECID Library) (submittedVersion, cc-by-nc-sa)
- Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona) (submittedVersion, public-domain)
- Max Planck Digital Library (submittedVersion)
- Edinburgh Research Explorer (University of Edinburgh) (submittedVersion, other-oa)
- MPG.PuRe (Max Planck Society) (submittedVersion)
- NORA - Norwegian Open Research Archives (submittedVersion, other-oa)
- arXiv (Cornell University)
- Funders
- National Science Foundation (DE-AC02-98CH10886, DEAC02-05CH11231, DE-SC0012704)
- U.S. Department of Energy (-AC02-05CH11231, DE‐SC0012704, 05CH11231, DEAC-02-98CH10886, DESC0014329, DESC0009959, DE AC02 05CH11231, -AC02-98 CH 10886, SC0012704., DESC0013718, DESC0010331, DESC0017860, DE-AC02-)
- National Aeronautics and Space Administration (DE-AC02-05CH11231, DE-SC0012704)
- Alfred P. Sloan Foundation (DE-AC02-05CH11231)
- Yale University (DE-AC02-05CH11231)
- Vanderbilt University
- Princeton University
- Ohio State University
- Harvard University
- University of Washington
- Johns Hopkins University
- University of Arizona
- Carnegie Mellon University
- University of Portsmouth
- New Mexico State University
- York University
- National Research Foundation (NRF-SGER 2014055950, ST/N000668/1)
- Deutsche Forschungsgemeinschaft (DE-AC02-05CH11231, MDM-2014-0369)
- Agence Nationale de la Recherche (ANR-11IDEX-0004-02, ANR-16-CE31-0021, ANR-10-LABX-63, ANR-11-IDEX, DE-AC02-05CH11231, IDEX-0004-02, ANR-10-LABX-0063, ANR-11-IDEX-0004, ANR-10, 10-LABX-63)
- Sejong University
- National Research Foundation of Korea (NRF-SGER 2014055950, DE-AC02-98CH10886)
- Ministry of Education, Science and Technology
- Office of Science (DE-AC-02-98CH10886, DESC0014329, DE-SC-0012704, DEAC02–05CH11231, AC02-05CH11231, DE-AC02, DESC0010331, SC0012704)
- College of Engineering, Michigan State University
- Science and Technology Facilities Council (ST/M001709/1, ST/N00180X/1, ST/K004719/1, DE-AC02-98CH10886, ST/N000668/1, ST/L00481X/1)
- Japan Society for the Promotion of Science (15K21733)
- Institut de Ciències del Cosmos (MDM-2014-0369)
- High Energy Physics (DE-SC0012704, DEAC02--05CH11231, DE-SC0014329)
- Brookhaven National Laboratory (SC0012704, AC-02-98CH10886, DE-AC02- 98CH10886, DE-AC02-05CH11231, DE- SC0012704)
- Lawrence Berkeley National Laboratory (AC02‐05CH11231, DE-AC02-05CH11231, DE-SC0012704, 05CH11231)
- FP7 Ideas: European Research Council (240117, 614030)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- galaxy clustering, baryon acoustic oscillations, BOSS, SDSS DR12, angular diameter distance, Hubble parameter, sound horizon, anisotropic clustering, large-scale structure, cosmological constraints
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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