The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
Carnegie Mellon University · Leibniz Institute for Astrophysics Potsdam · +57 more institutions
Abstract
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…
Citation impact
- FWCI
- 167.05
- Percentile
- 100%
- References
- 239
Authors
73Topics & keywords
- Physics
- Cosmic microwave background
- Dark energy
- Astrophysics
- Baryon acoustic oscillations
- Galaxy
- Redshift
- Redshift-space distortions
Funding
- NSNational Science FoundationAwards: DE-AC02-98CH10886, DE-AC02-05CH11231, DE-SC0012704
- UDU.S. Department of EnergyAwards: -AC02-05CH11231, 05CH11231, DE-SC0014329, AC02-98CH10886, SC0013718, DE-SC0009959, AC02-05CH11231, SC0012704, DE-AC02, DE-SC0013718, DE-AC02-05CH11231, DE-AC02-
- NANational Aeronautics and Space AdministrationAwards: DE-AC02-05CH11231, DE-SC0012704
- APAlfred P. Sloan FoundationAward: DE-AC02-05CH11231
- YUYale UniversityAward: DE-AC02-05CH11231
- VUVanderbilt University
- PUPrinceton University
- OSOhio State University
- HUHarvard University
- UOUniversity of Washington
- JHJohns Hopkins University
- UOUniversity of Arizona
- CMCarnegie Mellon University
- UOUniversity of Portsmouth
- NMNew Mexico State University
- YUYork University
- NRNational Research FoundationAwards: NRF-SGER 2014055950, ST/N000668/1
- DFDeutsche ForschungsgemeinschaftAwards: DE-AC02-05CH11231, MDM-2014-0369
- ANAgence Nationale de la RechercheAwards: ANR-11-IDEX-0004-02, ANR-10-LABX-63, ANR-11-IDEX, -11-IDEX-0004-02, DE-AC02-05CH11231, IDEX-0004-02, 11-IDEX-0004, 11-IDEX-0004-02, ANR-11-IDEX-0004, ANR-10, 10-LABX-63
- SUSejong University
- NRNational Research Foundation of KoreaAwards: NRF-SGER 2014055950, DE-AC02-98CH10886
- MOMinistry of Education, Science and Technology
- OOOffice of ScienceAwards: DE-AC02-98CH10886, AC02-05CH11231, -AC02-05CH11231, DE-AC02, DE-SC0014329, DE-SC0010331, SC0012704, DE-SC0012704
- COCollege of Engineering, Michigan State University
- SAScience and Technology Facilities CouncilAwards: ST/N000668/1, ST/K004719/1, ST/M001709/1, ST/N00180X/1, ST/M001709/1, ST/K004719/1, DE-AC02-98CH10886, ST/N000668/1, ST/L00481X/1
- IDInstitut de Ciències del CosmosAward: MDM-2014-0369
- HEHigh Energy PhysicsAwards: DE-SC0012704, DE-AC02-05CH11231, DE-SC0014329
- BNBrookhaven National LaboratoryAwards: SC0012704, DE-AC02-05CH11231, DE-AC02-98CH10886, AC02-98CH10886
- LBLawrence Berkeley National LaboratoryAwards: DE-AC02-05CH11231, DE-SC0012704, 05CH11231, AC02-05CH11231