{"paper":{"title":"Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Arun Kannawadi, Atsushi J. Nishizawa, Bau-ching Hsieh, Hironao Miyatake, Hitoshi Murayama, Ken Osato, Lauren A. MacArthur, Markus M. Rau, Masahiro Takada, Masamune Oguri, Masato Shirasaki, Masayuki Tanaka, Michael A. Strauss, Nate B. Lust, Paul A. Price, Philip J. Tait, Rachel Mandelbaum, Robert Armstrong, Robert H. Lupton, Roohi Dalal, Ryuichi Takahashi, Satoshi Miyazaki, Shiang-Yu Wang, Sunao Sugiyama, Surhud More, Takahiro Nishimichi, Takashi Hamana, Tianqing Zhang, Tomomi Sunayama, Wentao Luo, Xiangchong Li, Yosuke Kobayashi, Yuki Okura, Yutaka Komiyama","submitted_at":"2023-04-03T03:37:04Z","abstract_excerpt":"We present cosmology results from a blinded joint analysis of cosmic shear, $\\xi_{\\pm}(\\vartheta)$, galaxy-galaxy weak lensing, $\\Delta\\!\\Sigma(R)$, and projected galaxy clustering, $w_{\\rm p}(R)$, measured from the Hyper Suprime-Cam three-year (HSC-Y3) shape catalog and the Sloan Digital Sky Survey (SDSS) DR11 spectroscopic galaxy catalog - a 3$\\times$2pt cosmology analysis. We define luminosity-cut samples of SDSS galaxies to serve as the tracers of $w_{\\rm p}$ and as the lens samples for $\\Delta\\!\\Sigma$ in three spectroscopic redshift bins spanning the range $0.15<z<0.7$. For the $\\xi_{\\pm"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2304.00704","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2304.00704/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}