Showing 1–17 of 17 results
/ Date/ Name
Aug 25, 2021Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$Apr 3, 2023Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power SpectraApr 3, 2023Hyper Suprime-Cam Year 3 Results: Measurements of Clustering of SDSS-BOSS Galaxies, Galaxy-Galaxy Lensing and Cosmic ShearJul 2, 2025Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction ModelJul 2, 2025Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-CalibrationApr 3, 2023Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias ModelSep 22, 2023Optical Cluster Cosmology with SDSS redMaPPer clusters and HSC-Y3 lensing measurementsDec 6, 2022A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing AnalysisNov 29, 2022Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogueJan 18, 2024A Systematic Search of Distant Superclusters with the Subaru Hyper Suprime-Cam SurveyApr 3, 2023Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation FunctionsApr 11, 2023The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological ParametersNov 18, 2024Miscentering of Optical Galaxy Clusters Based on Sunyaev-Zeldovich CounterpartsApr 3, 2023Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo ModelDec 19, 2024Mitigating Nonlinear Systematics in Weak Lensing Surveys: The Bernardeau-Nishimichi-Taruya ApproachJun 29, 2021Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parametersApr 11, 2023The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth