Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing

作者: J. Colin Hill , Jia Liu , Kevin M. Huffenberger , Gabriela A. Marques

DOI: 10.3847/1538-4357/ABC003

关键词: PlanckPhysicsGalaxyPhotometric redshiftObservational cosmologyCosmic microwave backgroundAstrophysicsCosmologyRedshiftWeak gravitational lensing

摘要: Cross-correlations between galaxy weak lensing (WL) and Cosmic Microwave Background (CMB) are a powerful tool to probe matter fluctuations at intermediate redshifts detect residual systematics in either probe. In this paper, we study the cross-correlation of WL from Hyper Suprime-Cam Subaru Strategic Program (HSC) first data release CMB final Planck release, for HSC source galaxies 0.3< z < 1.5. is deepest Stage-III survey, provides both great opportunity high-redshift universe new challenges related its exceptionally high density, such as blending. The signal measured significance level 3.1$\sigma$. amplitude our best-fit model with respect 2018 cosmology $A = 0.81\pm 0.25$, consistent $A=1$. Our result also previous studies using different surveys. We perform tests $B$-modes, point-spread-function, photometric redshift errors, thermal Sunyaev-Zel'dovich leakage, find no significant evidence systematics.

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