Cosmological inference from an emulator based halo model. II. Joint analysis of galaxy-galaxy weak lensing and galaxy clustering from HSC-Y1 and SDSS Article Swipe

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Hironao Miyatake , Sunao Sugiyama , Masahiro Takada , Takahiro Nishimichi , Masato Shirasaki , Yosuke Kobayashi , Rachel Mandelbaum , Surhud More , Masamune Oguri , Ken Osato , Youngsoo Park , Ryuichi Takahashi , Jean Coupon , Chiaki Hikage , Bau-Ching Hsieh , Alexie Leauthaud , Xiangchong Li , Wentao Luo , Robert H. Lupton , Satoshi Miyazaki , Hitoshi Murayama , Atsushi J. Nishizawa , P. A. Price , Melanie Simet , Joshua S. Speagle , Michael A. Strauss , Masayuki Tanaka , Naoki Yoshida ·

YOU? · · 2022 · Open Access · · DOI: https://doi.org/10.1103/physrevd.106.083520

Here, we present high-fidelity cosmology results from a blinded joint analysis of galaxy-galaxy weak lensing (ΔΣ) and projected galaxy clustering (w_p) measured from the Hyper Suprime-Cam Year-1 (HSC-Y1) data and spectroscopic Sloan Digital Sky Survey (SDSS) galaxy catalogs in the redshift range 0.15 < z < 0.7. We define luminosity-limited samples of SDSS galaxies to serve as the tracers of w_p in three spectroscopic redshift bins, and as the lens samples for ΔΣ. For the ΔΣ measurements, we select a single sample of 4×10⁶ source galaxies over 140 deg² from HSC-Y1 with photometric redshifts (photo z) greater than 0.75, enabling a better handle of photo- z errors by comparing the ΔΣ amplitudes for the three lens redshift bins. The deep, high-quality HSC-Y1 data enable significant detections of the ΔΣ signals, with integrated signal-to-noise ratio S/N ~ 15 in the range 3 ≤ R/[h^–1 Mpc] ≤ 30 for the three lens samples, despite the small area coverage. For cosmological parameter inference, we use an input galaxy-halo connection model built on the dark emulator package (which uses an ensemble set of high-resolution N-body simulations and enables fast, accurate computation of the clustering observables) with a halo occupation distribution that includes nuisance parameters to marginalize over modeling uncertainties. We model the ΔΣ and wp measurements on scales from R≃3 and 2h^–1 Mpc , respectively, up to 30 h^–1 Mpc (therefore excluding the baryon acoustic oscillations information) assuming a flat Λ CDM cosmology, marginalizing over about 20 nuisance parameters and demonstrating the robustness of our results to them. With various tests using mock catalogs described in Miyatake et al. [preceding paper, Phys. Rev. D 106, 083519 (2022)], we show that any bias in the clustering amplitude S₈ ≡ σ₈(Ω_m/0.3)^0.5 due to uncertainties in the galaxy-halo connection is less than ~ 50 % of the statistical uncertainty of S₈, unless the assembly biaseffect is unexpectedly large. Our best-fit models have S₈ = 0.795$_{-0.042}^{+0.049}$ (mode and 68% credible interval) for the flat Λ CDM model; we find tighter constraints on the quantity S₈(α = 0.17)≡σ₈(Ω_m/0.3)^0.17 = 0.745$_{-0.031}^{+0.039}$.

Related Topics

Physics

Astrophysics

Galaxy

Halo (Optical Phenomenon)

Cosmology

Sigma

Astronomy

Concepts

Physics Astrophysics Galaxy Redshift Halo Cosmology Sigma Weak gravitational lensing Luminosity Astronomy

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Type: preprint
Language: en
Landing Page: https://doi.org/10.1103/physrevd.106.083520
OA Status: green
References: 134
Related Works: 10
OpenAlex ID: https://openalex.org/W4225694764

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DOI: https://doi.org/10.1103/physrevd.106.083520

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Title: Cosmological inference from an emulator based halo model. II. Joint analysis of galaxy-galaxy weak lensing and galaxy clustering from HSC-Y1 and SDSS

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Type: preprint

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Language: en

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Publication year: 2022

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Publication date: 2022-10-21

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Authors: Hironao Miyatake, Sunao Sugiyama, Masahiro Takada, Takahiro Nishimichi, Masato Shirasaki, Yosuke Kobayashi, Rachel Mandelbaum, Surhud More, Masamune Oguri, Ken Osato, Youngsoo Park, Ryuichi Takahashi, Jean Coupon, Chiaki Hikage, Bau-Ching Hsieh, Alexie Leauthaud, Xiangchong Li, Wentao Luo, Robert H. Lupton, Satoshi Miyazaki, Hitoshi Murayama, Atsushi J. Nishizawa, P. A. Price, Melanie Simet, Joshua S. Speagle, Michael A. Strauss, Masayuki Tanaka, Naoki Yoshida

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Landing page: https://doi.org/10.1103/physrevd.106.083520

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OA URL: https://www.osti.gov/biblio/1992466

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Concepts: Physics, Astrophysics, Galaxy, Redshift, Halo, Cosmology, Sigma, Weak gravitational lensing, Luminosity, Astronomy

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Cited by: 0

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References (count): 134

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