The extended Baryon Oscillation Spectroscopic Survey: a cosmological forecast

Autor: Gong-Bo Zhao, Sarah Shandera, Donald P. Schneider, Francisco Prada, Jean-Paul Kneib, Yuting Wang, Timothée Delubac, Christophe Yèche, Xu Zhou, Kyle S. Dawson, H. Y. Zhang, Andres Meza, Dandan Wang, Nathalie Palanque-Delabrouille, Graziano Rossi, Ashley J. Ross, Alireza Hojjati, Hee-Jong Seo, Yuecheng Zhang, Levon Pogosian, Cameron K. McBride, Hu Zou, Adam D. Myers, Johan Comparat, Kazuya Koyama, Pengyuan Gao, Will J. Percival, Charling Tao, Jeffrey A. Newman, Fangzhou Zhu, Joel R. Brownstein
Přispěvatelé: Key Laboratory for Liquid-Solid Structural Evolution and Processing of Materials, Shandong University, Department of Electrical and Computer Engineering [Minneapolis] (ECE), University of Minnesota [Twin Cities] (UMN), University of Minnesota System-University of Minnesota System, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Departamento de FisicaTeorica e IFT-UAM/CSIC, Universidad Autónoma de Madrid (UAM), EPFL Laboratoire d’astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Institute of Cosmology & Gravitation, Dennis Sciama Building, University of Portsmouth, Department of Physics and Astronomy [Pittsburgh], University of Pittsburgh (PITT), Pennsylvania Commonwealth System of Higher Education (PCSHE)-Pennsylvania Commonwealth System of Higher Education (PCSHE), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Universidad Autonoma de Madrid (UAM)
Jazyk: angličtina
Rok vydání: 2016
Předmět:
Cosmology and Gravitation
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
NEUTRINO MASS
01 natural sciences
ACOUSTIC-OSCILLATIONS
symbols.namesake
ST/K00090/1
0103 physical sciences
Planck
dark energy
010303 astronomy & astrophysics
Weak gravitational lensing
STFC
Astrophysics::Galaxy Astrophysics
Physics
010308 nuclear & particles physics
Oscillation
RCUK
CONSTRAINTS
Astronomy and Astrophysics
Quasar
FOREST
Galaxy
Baryon
large scale structure of Universe
GALAXIES
QUASARS
DATA SETS
Space and Planetary Science
SDSS-III
NON-GAUSSIANITY
symbols
Dark energy
astro-ph.CO
DIGITAL SKY SURVEY
DARK ENERGY
large-scale structure of Universe
Neutrino
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Astrophysics - Cosmology and Nongalactic Astrophysics
Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2016, 457 (3), pp.2377--2390. ⟨10.1093/mnras/stw135⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 457 (3), pp.2377--2390. ⟨10.1093/mnras/stw135⟩
Zhao, G-B, Wang, Y, Ross, A J, Shandera, S, Percival, W J, Dawson, K S, Kneib, J-P, Myers, A D, Brownstein, J R, Comparat, J, Delubac, T, Gao, P, Hojjati, A, Koyama, K, McBride, C K, Meza, A, Newman, J A, Palanque-Delabrouille, N, Pogosian, L, Prada, F, Rossi, G, Schneider, D P, Seo, H-J, Tao, C, Wang, D, Yèche, C, Zhang, H, Zhang, Y, Zhou, X, Zhu, F & Zou, H 2016, ' The extended Baryon Oscillation Spectroscopic Survey (eBOSS) : a cosmological forecast ', MNRAS, vol. 457, no. 3, pp. 2377-2390 . https://doi.org/10.1093/mnras/stw135
ISSN: 0035-8711
1365-2966
Popis: We present a science forecast for the eBOSS survey, part of the SDSS-IV project, which is a spectroscopic survey using multiple tracers of large-scale structure, including luminous red galaxies (LRGs), emission line galaxies (ELGs) and quasars (both as a direct probe of structure and through the Ly-$\alpha$ forest). Focusing on discrete tracers, we forecast the expected accuracy of the baryonic acoustic oscillation (BAO), the redshift-space distortion (RSD) measurements, the $f_{\rm NL}$ parameter quantifying the primordial non-Gaussianity, the dark energy and modified gravity parameters. We also use the line-of-sight clustering in the Ly-$\alpha$ forest to constrain the total neutrino mass. We find that eBOSS LRGs ($0.60.6$), ELGs ($0.6
Comment: 15 pages, 9 figures, 6 tables; matches the published version on MNRAS
Databáze: OpenAIRE