Cosmology from a joint analysis of second- and third-order shear statistics with Subaru Hyper Suprime-Cam Year 3 data
Year: 2025
Type: article
Abstract: We present a joint cosmological analysis of the two-point correlation function and the aperture-mass skewness measured from the Year 3 data of the Hyper Suprime-Cam Subaru Strategic Program (HSC-Y3). The aperture-mass skewness is a compressed representation of three-point shear information, designed to capture non-Gaussian features while keeping the data vector computationally tractable. We find that including the aperture-mass skewness improves the $S_8$-$Ω_m$ figure of merit by 80% compared to the 2PCF-only case, primarily due to the breaking of degeneracies. Our joint analysis yields a constraint of $S_8=0.736\pm0.020$, which is slightly lower than the two-point-only result and increases the tension with Planck 2018 to 3.2$σ$ in the $S_8$-$Ω_m$ plane. The two- and three-point statistics are found to be internally consistent across redshift bins and angular scales, and we detect no significant intrinsic alignment signal. We also explore extensions to the $w$CDM model and find no evidence for deviations from a cosmological constant. This work demonstrates the feasibility and scientific value of incorporating third-order shear statistics into weak lensing cosmology and provides a practical pathway for similar analyses in future Stage-IV surveys such as LSST, Euclid, and Roman.
DOI: 10.1103/6wk9-q5gh
Authors: Sunao Sugiyama, Rafael C. H. Gomes, Bhuvnesh Jain
Institution: University of Pennsylvania
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Funders: National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Kavli Foundation, Bread and Roses Community Fund, Princeton University, Ministry of Education, Culture, Sports, Science and Technology, Cabinet Office, Government of Japan, National Astronomical Observatory of Japan, High Energy Accelerator Research Organization, Toray Science Foundation, Jet Propulsion Laboratory, Japan Society for the Promotion of Science, Japan Science and Technology Agency
OpenAlex ID: W4417268296
