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Abstract
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 ($0.6z 0.6$), ELGs ($0.6z($0.6z
Original language | English |
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Pages (from-to) | 2377-2390 |
Number of pages | 14 |
Journal | MNRAS |
Volume | 457 |
Issue number | 3 |
Early online date | 10 Feb 2016 |
DOIs | |
Publication status | Published - 11 Apr 2016 |
Keywords
- astro-ph.CO
- RCUK
- STFC
- ST/K00090/1
- dark energy
- large scale structure of Universe
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