The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
- Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
- Max Planck Institute for Extraterrestrial Physics, Garching (Germany); Univ. Observatory Munich (Germany)
- Carnegie Mellon Univ., Pittsburgh, PA (United States). Dept. of Physics and McWilliams Center for Cosmology
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation; The Ohio State Univ., Columbus, OH (United States). Center for Cosmology and Astro-Particle Physics
- Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy
- Autonomous Univ. of Madrid (Spain). Inst. of Theoretical Physics; Leibniz Inst. for Astrophysics Potsdam (Germany)
- Univ. of Barcelona (Spain). Inst. of Cosmic Sciences
- Harvard Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Leibniz Inst. for Astrophysics Potsdam (Germany); Univ. of California, Berkeley, CA (United States). Dept. of Physics and Astronomy
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation
- Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy; Campus of International Excellence UAM, Madrid (Spain); Inst. of Astrophysics of Andalucia, Granada (Spain)
- Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy; Campus of International Excellence UAM, Madrid (Spain); Autonomous Univ. of Madrid (Spain). Dept. of Theoretical Physics
- Ohio Univ., Athens, OH (United States). Dept. of Physics and Astronomy
- New York Univ., NY (United States). Cetner for Cosmology and Particle Physics
- Univ. of St. Andrews, Scotland (United Kingdom). School of Physics and Astronomy
- Carnegie Mellon Univ., Pittsburgh, PA (United States). Dept. of Physics and McWilliams Center for Cosmology; Autonomous National Univ. of Mexico, Mexico DF (Mexico)
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Chinese Academy of Sciences (CAS), Beijing (China). National Astronomy Observatories
The cosmological information contained in anisotropic galaxy clustering measurements can often be compressed into a small number of parameters whose posterior distribution is well described by a Gaussian. Here, we present a general methodology to combine these estimates into a single set of consensus constraints that encode the total information of the individual measurements, taking into account the full covariance between the different methods. We also illustrate this technique by applying it to combine the results obtained from different clustering analyses, including measurements of the signature of baryon acoustic oscillations and redshift-space distortions, based on a set of mock catalogues of the final SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Our results show that the region of the parameter space allowed by the consensus constraints is smaller than that of the individual methods, highlighting the importance of performing multiple analyses on galaxy surveys even when the measurements are highly correlated. Our paper is part of a set that analyses the final galaxy clustering data set from BOSS. The methodology presented here is used in Alam et al. to produce the final cosmological constraints from BOSS.
- Research Organization:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Grant/Contract Number:
- SC00112704
- OSTI ID:
- 1336116
- Report Number(s):
- BNL-112565-2016-JA; KA2301020
- Journal Information:
- Monthly Notices of the Royal Astronomical Society, Vol. 464, Issue 2; ISSN 0035-8711
- Publisher:
- Royal Astronomical SocietyCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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