The Hyper Suprime-Cam SSP Survey: Overview and survey design

H. Aihara(The University of Tokyo), N. Arimoto(The Graduate University for Advanced Studies, SOKENDAI), R. Armstrong(Princeton University), S. Arnouts(Centre National de la Recherche Scientifique), Neta A. Bahcall(Princeton University), Steven J. Bickerton(Orbital ATK (United States)), James Bosch(Princeton University), Kevin Bundy(Kavli Institute for the Physics and Mathematics of the Universe), P. Capak(California Institute of Technology), J. H. H. Chan(Institute of Astronomy and Astrophysics, Academia Sinica), Masashi Chiba(Tohoku University), Yôko Tanaka(University of Geneva), Yousuke Utsumi(University of Arizona), Junko Furusawa(Tokyo Keizai University), Akira Konno(Subaru (Japan)), N. Katayama, Jenny E. Greene(The University of Tokyo), Keiichi Umetsu(National Astronomical Observatory of Japan), Paul T. P. Ho(National Astronomical Observatory of Japan), Johnny P. Greco(National Tsing Hua University), Ryo Higuchi(Princeton University), Masaomi Tanaka(Princeton University), Philip J. Tait(Princeton University), Ikuru Iwata(Princeton University), James E. Gunn(National Astronomical Observatory of Japan), Takashi Hamana(The University of Tokyo), Yuichi Harikane(National Taiwan Normal University), K. Iwasawa(Subaru (Japan)), Masayuki Tanaka(National Astronomical Observatory of Japan), Yasuhiro Hashimoto(National Astronomical Observatory of Japan), Anton T. Jaelani(Nicolaus Copernicus Astronomical Center), Takashi Hattori(The University of Tokyo), Satoshi Kawanomoto(Kavli Institute for the Physics and Mathematics of the Universe), Masao Hayashi(Institute of Astronomy and Astrophysics, Academia Sinica), Yusuke Hayashi(Institute of Astronomy and Astrophysics, Academia Sinica), N. Suzuki(National Taiwan Normal University), Kenneth C. Wong(Kavli Institute for the Physics and Mathematics of the Universe), Bau-Ching Hsieh(National Astronomical Observatory of Japan), Chiaki Hikage(The Graduate University for Advanced Studies, SOKENDAI), Tomonori Usuda(Osaka Sangyo University), Nozomu Tominaga(Institució Catalana de Recerca i Estudis Avançats), Kuiyun Huang(The Graduate University for Advanced Studies, SOKENDAI), Hung-Yu Jian(Tohoku University), Surhud More(Institute of Astronomy and Astrophysics, Academia Sinica), Song Huang(National Astronomical Observatory of Japan), Hiroyuki Ikeda(National Institutes of Natural Sciences), Haruka Kusakabe(The Graduate University for Advanced Studies, SOKENDAI), Masatoshi Imanishi(Kavli Institute for the Physics and Mathematics of the Universe), Akio Inoue(National Astronomical Observatory of Japan), Hisakazu Uchiyama(Tokyo University of Technology), Hitomi Yamanoi(Stony Brook University), Hiroshi Karoji(National Astronomical Observatory of Japan), Yukiko Kamata(The University of Tokyo), S. H. Suyu(The Graduate University for Advanced Studies, SOKENDAI), Issha Kayo(The University of Tokyo), Nobunari Kashikawa(Subaru (Japan)), Alexie Leauthaud(The Graduate University for Advanced Studies, SOKENDAI), Atsunori Yonehara(The University of Tokyo), Sogo Mineo(Kavli Institute for the Physics and Mathematics of the Universe), Jin Koda(Subaru (Japan)), Yoshiki Matsuoka(Institute of Astronomy and Astrophysics, Academia Sinica), Shintaro Koshida(Institute of Astronomy and Astrophysics, Academia Sinica), Michitaro Koike(Princeton University), Takashi Kojima(Carnegie Mellon University), Tomotsugu Goto(National Astronomical Observatory of Japan), Yutaka Komiyama(Princeton University), Elinor Medezinski(National Astronomical Observatory of Japan), Yoshiki Toba(Hiroshima University), Anupreeta More(Jet Propulsion Laboratory), Yasushi Suto(The Graduate University for Advanced Studies, SOKENDAI), Rachel Mandelbaum(National Tsing Hua University), Yusei Koyama(Kavli Institute for the Physics and Mathematics of the Universe), Shoken M. Miyama(Kavli Institute for the Physics and Mathematics of the Universe), Wei-Hao Wang(Kavli Institute for the Physics and Mathematics of the Universe), Lee, C.-H.(National Astronomical Observatory of Japan), Shiro Mukae(Kavli Institute for the Physics and Mathematics of the Universe), Lihwai Lin(The University of Tokyo), Yen‐Ting Lin(Kavli Institute for the Physics and Mathematics of the Universe), Yuma Sugahara(Lawrence Berkeley National Laboratory), Robert H. Lupton(Ehime University), Ryoma Murata(Subaru (Japan)), M. Tanaka(Ehime University), Naoshi Sugiyama(Kavli Institute for the Physics and Mathematics of the Universe), Hiroko Niikura(Nagoya University), Hironao Miyatake(National Astronomical Observatory of Japan), Tomohisa Uchida(Kavli Institute for the Physics and Mathematics of the Universe), Naoyuki Tamura(National Astronomical Observatory of Japan), Y. Urata(Hiroshima University), Satoshi Miyazaki(Shanghai Astronomical Observatory), Rieko Momose(Brookhaven National Laboratory), Yoshihiko Yamada(The University of Tokyo), Joshua S. Speagle(Subaru (Japan)), Yuichi Terashima(The Graduate University for Advanced Studies, SOKENDAI), Atsushi J. Nishizawa(The University of Tokyo), Sakurako Okamoto(Kavli Institute for the Physics and Mathematics of the Universe), Yuki Moritani(Princeton University), Takashi J. Moriya(Subaru (Japan)), Hitoshi Murayama(University of Pennsylvania), Tomoki Morokuma(Saint Mary's University), Sherry Yeh(The University of Tokyo), Michael A. Strauss(National Taiwan Normal University), Tohru Nagao(Kavli Institute for the Physics and Mathematics of the Universe), Yuki Okura(National Astronomical Observatory of Japan), Yoshiyuki Obuchi(Kavli Institute for the Physics and Mathematics of the Universe), Masamune Oguri(University of California, Riverside), Tsuyoshi Terai(Harvard University), Masahiro Takada(Princeton University), Fumiaki Nakata(Princeton University), Tae‐Soo Pyo(The University of Tokyo), Mana Niida(Kavli Institute for the Physics and Mathematics of the Universe), Shiang‐Yu Wang(The University of Tokyo), David N. Spergel(Institute of Astronomy and Astrophysics, Academia Sinica), Edwin L. Turner(Kavli Institute for the Physics and Mathematics of the Universe), Yukie Oishi(Subaru (Japan)), N. Okabe(Kavli Institute for the Physics and Mathematics of the Universe), Tadafumi Takata(The Graduate University for Advanced Studies, SOKENDAI), Yoshiaki Ono(Kavli Institute for the Physics and Mathematics of the Universe), Andy D. Goulding(High Energy Accelerator Research Organization), Fumihiro Uraguchi(National Astronomical Observatory of Japan), Hiroki Fujimori(National Astronomical Observatory of Japan), Motohiro Enoki(Subaru (Japan)), Masato Onodera(Subaru (Japan)), Masafusa Onoue(Ehime University), Eiichi Egami(Institute of Astronomy and Astrophysics, Academia Sinica), Ken Osato(Konan University), Melanie Simet(The University of Tokyo), Masami Ouchi(Kavli Institute for the Physics and Mathematics of the Universe), P. A. Price(High Energy Accelerator Research Organization), Kazuhiro Shimasaku(The Graduate University for Advanced Studies, SOKENDAI), Kiyoto Yabe(Institute of Astronomy and Astrophysics, Academia Sinica), Seiji Fujimoto(National Astronomical Observatory of Japan), J. D. Silverman(National Central University), Atsushi Shimono(The Graduate University for Advanced Studies, SOKENDAI), Masao Sako(Hiroshima University), Marcin Sawicki(Institute of Astronomy and Astrophysics, Academia Sinica), F. Finet(Institute of Astronomy and Astrophysics, Academia Sinica), Masato Shirasaki(Institute of Astronomy and Astrophysics, Academia Sinica), K. G. Hełminiak(Kavli Institute for the Physics and Mathematics of the Universe), Takatoshi Shibuya(National Astronomical Observatory of Japan), Hisanori Furusawa(National Astronomical Observatory of Japan), Naoki Yasuda(Kavli Institute for the Physics and Mathematics of the Universe), Jean Coupon(Subaru (Japan)), Jun Toshikawa(Kyoto Sangyo University), Suraphong Yuma(Mahidol University)
Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona)
January 1, 2018
Cited by 776

Abstract

Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2-m Subaru telescope on the summit of Mauna Kea in Hawaii. A team of scientists from Japan, Taiwan, and Princeton University is using HSC to carry out a 300-night multi-band imaging survey of the high-latitude sky. The survey includes three layers: the Wide layer will cover 1400 deg2 in five broad bands (grizy), with a 5 σ point-source depth of r ≈ 26. The Deep layer covers a total of 26 deg2 in four fields, going roughly a magnitude fainter, while the UltraDeep layer goes almost a magnitude fainter still in two pointings of HSC (a total of 3.5 deg2). Here we describe the instrument, the science goals of the survey, and the survey strategy and data processing. This paper serves as an introduction to a special issue of the Publications of the Astronomical Society of Japan, which includes a large number of technical and scientific papers describing results from the early phases of this survey.


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