Cosmology with galaxy–galaxy lensing on non-perturbative scales: emulation method and application to BOSS LOWZ

Wibking, Benjamin D.; Weinberg, David H.; Salcedo, Andrés N.; Wu, Hao-Yi; Singh, Sukhdeep; Rodríguez-Torres, Sergio; Garrison, Lehman H.; Eisenstein, Daniel J.

doi:10.1093/mnras/stz3423

Title: Cosmology with galaxy–galaxy lensing on non-perturbative scales: emulation method and application to BOSS LOWZ

Journal Article · 17 December 2019 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stz3423 · OSTI ID:1592788

^[1]; Weinberg, David H. ^[1];

^[1];

^[1]; Singh, Sukhdeep ^[2]; Rodríguez-Torres, Sergio ^[3];

^[4]; Eisenstein, Daniel J. ^[4]

The Ohio State Univ., Columbus, OH (United States)
Univ. of California, Berkeley, CA (United States)
Universidad Autónoma de Madrid (UAM) Madrid (Spain); Instituto de Astrofisica de Canarias (Spain)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)

We describe our non-linear emulation (i.e. interpolation) framework that combines the halo occupation distribution (HOD) galaxy bias model with N-body simulations of non-linear structure formation, designed to accurately predict the projected clustering and galaxy–galaxy lensing signals from luminous red galaxies in the redshift range 0.16 < z < 0.36 on comoving scales 0.6 < rp < 30 $$h^{-1} \, \text{Mpc}$$. The interpolation accuracy is ≲ 1–2 percent across the entire physically plausible range of parameters for all scales considered. We correctly recover the true value of the cosmological parameter S8 = (σ8/0.8228)(Ωm/0.3107)0.6 from mock measurements produced via subhalo abundance matching (SHAM)-based light-cones designed to approximately match the properties of the SDSS LOWZ galaxy sample. Applying our model to Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 14 (DR14) LOWZ galaxy clustering and galaxy-shear cross-correlation measurements made with Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8) imaging, we perform a prototype cosmological analysis marginalizing over wCDM cosmological parameters and galaxy HOD parameters. We obtain a 4.4 percent measurement of S8 = 0.847 ± 0.037, in 3.5σ tension with the Planck cosmological results of 1.00 ± 0.02. We discuss the possibility of underestimated systematic uncertainties or astrophysical effects that could explain this discrepancy.

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Research Organization:: Krell Institute, Ames, IA (United States); Harvard Univ., Cambridge, MA (United States)

Sponsoring Organization:: USDOE Office of Science (SC); USDOE National Nuclear Security Administration (NNSA)

Grant/Contract Number:: FG02-97ER25308; SC0013718

OSTI ID:: 1592788

Alternate ID(s):: OSTI ID: 1800926

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 2; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 35 works

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