Combined full shape analysis of BOSS galaxies and eBOSS quasars using an iterative emulator
Richard Neveux, Etienne Burtin, Vanina Ruhlmann-Kleider, Arnaud de, Mattia, Agne Semenaite, Kyle S. Dawson, Axel de la Macorra, Will J. Percival,, Graziano Rossi, Donald P. Schneider, Gong-Bo Zhao

TL;DR
This paper introduces a novel cosmological analysis method that directly explores parameter space using an iterative emulator, improving constraints from galaxy and quasar clustering data without relying on fixed templates.
Contribution
It develops an iterative Gaussian process emulator for full-shape clustering analysis, enabling direct cosmology parameter space exploration and reducing computational costs.
Findings
Constraints on cosmological parameters from combined eBOSS and BOSS data.
Detection of a 3.1σ discrepancy in quasar data compared to Planck.
Validation of the method with N-body simulation mocks.
Abstract
Standard full-shape clustering analyses in Fourier space rely on a fixed power spectrum template, defined at the fiducial cosmology used to convert redshifts into distances, and compress the cosmological information into the Alcock-Paczynski parameters and the linear growth rate of structure. In this paper, we propose an analysis method that operates directly in the cosmology parameter space and varies the power spectrum template accordingly at each tested point. Predictions for the power spectrum multipoles from the TNS model are computed at different cosmologies in the framework of . Applied to the final eBOSS QSO and LRG samples together with the low-z DR12 BOSS galaxy sample, our analysis results in a set of constraints on the cosmological parameters , , , and . To reduce the number of computed models, we…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories · Astronomy and Astrophysical Research
