@article{97c593f08a3e40dc8724e99bad692cfb,
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",
abstract = "We present high-fidelity cosmology results from a blinded joint analysis of galaxy-galaxy weak lensing (Δς) and projected galaxy clustering (wp) 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",
author = "Hironao Miyatake and Sunao Sugiyama and Masahiro Takada and Takahiro Nishimichi and Masato Shirasaki and Yosuke Kobayashi and Rachel Mandelbaum and Surhud More and Masamune Oguri and Ken Osato and Youngsoo Park and Ryuichi Takahashi and Jean Coupon and Chiaki Hikage and Hsieh, {Bau Ching} and Yutaka Komiyama and Alexie Leauthaud and Xiangchong Li and Wentao Luo and Lupton, {Robert H.} and Satoshi Miyazaki and Hitoshi Murayama and Nishizawa, {Atsushi J.} and Price, {Paul A.} and Melanie Simet and Speagle, {Joshua S.} and Strauss, {Michael A.} and Masayuki Tanaka and Naoki Yoshida",
note = "Funding Information: We would like to thank Ryoma Murata for his contribution during the early phase of this work. This work was supported in part by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan, and JSPS KAKENHI Grants No. JP15H03654, No. JP15H05887, No. JP15H05893, No. JP15H05896, No. JP15K21733, No. JP17H01131, No. JP17K14273, No. JP18H04350, No. JP18H04358, No. JP19H00677, No. JP19K14767, No. JP20H00181, No. JP20H01932, No. JP20H04723, No. JP20H05850, No. JP20H05855, No. JP20H05856, No. JP20H05861, No. JP21J00011, No. JP21J10314, No. JP21H01081, and No. JP21H05456 by Japan Science and Technology Agency (JST) CREST JPMHCR1414, by JST AIP Acceleration Research Grant No. JP20317829, Japan, and by Basic Research Grant (Super AI) of Institute for AI and Beyond of the University of Tokyo. H. M. and M. Si. were supported by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. S. S. is supported by International Graduate Program for Excellence in Earth-Space Science (IGPEES), World-leading Innovative Graduate Study (WINGS) Program, the University of Tokyo. Y. K. was supported by the Advanced Leading Graduate Course for Photon Science at the University of Tokyo. K. O. is supported by JSPS Research Fellowships for Young Scientists. R. M. is supported by a grant from the Simons Foundation (Simons Investigator in Astrophysics, Grant No. 620789). A. L. is supported by the U.D Department of Energy, Office of Science, Office of High Energy Physics under Award No. DE-SC0019301. J. S. S. acknowledges support as a Banting and Dunlap Fellow. The Hyper Suprime-Cam (HSC) collaboration includes the astronomical communities of Japan and Taiwan, and Princeton University. The HSC instrumentation and software were developed by the National Astronomical Observatory of Japan (NAOJ), the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), the University of Tokyo, the High Energy Accelerator Research Organization (KEK), the Academia Sinica Institute for Astronomy and Astrophysics in Taiwan (ASIAA), and Princeton University. Funding was contributed by the FIRST program from Japanese Cabinet Office, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), Japan Science and Technology Agency (JST), the Toray Science Foundation, NAOJ, Kavli IPMU, KEK, ASIAA, and Princeton University. This paper makes use of software developed for the Large Synoptic Survey Telescope. We thank the LSST Project for making their code available as free software at . The Pan-STARRS1 Surveys (PS1) have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg, and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen{\textquoteright}s University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under Grant No. AST-1238877, the University of Maryland, and Eotvos Lorand University (ELTE) and the Los Alamos National Laboratory. This paper uses in part data collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by Subaru Telescope and Astronomy Data Center at National Astronomical Observatory of Japan. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. Publisher Copyright: {\textcopyright} 2022 American Physical Society.",
year = "2022",
month = oct,
day = "15",
doi = "10.1103/PhysRevD.106.083520",
language = "English (US)",
volume = "106",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "8",
}