First data release of the Hyper Suprime-Cam Subaru Strategic Program

Hiroaki Aihara; Robert Armstrong; Steven Bickerton; James Bosch; Jean Coupon; Hisanori Furusawa; Yusuke Hayashi; Hiroyuki Ikeda; Yukiko Kamata; Hiroshi Karoji; Satoshi Kawanomoto; Michitaro Koike; Yutaka Komiyama; Dustin Lang; Robert H. Lupton; Sogo Mineo; Hironao Miyatake; Satoshi Miyazaki; Tomoki Morokuma; Yoshiyuki Obuchi; Yukie Oishi; Yuki Okura; Paul A. Price; Tadafumi Takata; Manobu M. Tanaka; Masayuki Tanaka; Yoko Tanaka; Tomohisa Uchida; Fumihiro Uraguchi; Yousuke Utsumi; Shiang Yu Wang; Yoshihiko Yamada; Hitomi Yamanoi; Naoki Yasuda; Nobuo Arimoto; Masashi Chiba; Francois Finet; Hiroki Fujimori; Seiji Fujimoto; Junko Furusawa; Tomotsugu Goto; Andy Goulding; James E. Gunn; Yuichi Harikane; Takashi Hattori; Masao Hayashi; Krzysztof G. Helminiak; Ryo Higuchi; Chiaki Hikage; Paul T.P. Ho; Bau Ching Hsieh; Kuiyun Huang; Song Huang; Masatoshi Imanishi; Ikuru Iwata; Anton T. Jaelani; Hung Yu Jian; Nobunari Kashikawa; Nobuhiko Katayama; Takashi Kojima; Akira Konno; Shintaro Koshida; Haruka Kusakabe; Alexie Leauthaud; Chien Hsiu Lee; Lihwai Lin; Yen Ting Lin; Rachel Mandelbaum; Yoshiki Matsuoka; Elinor Medezinski; Shoken Miyama; Rieko Momose; Anupreeta More; Surhud More; Shiro Mukae; Ryoma Murata; Hitoshi Murayama; Tohru Nagao; Fumiaki Nakata; Mana Niida; Hiroko Niikura; Atsushi J. Nishizawa; Masamune Oguri; Nobuhiro Okabe; Yoshiaki Ono; Masato Onodera; Masafusa Onoue; Masami Ouchi; Tae Soo Pyo; Takatoshi Shibuya; Kazuhiro Shimasaku; Melanie Simet; Joshua Speagle; David N. Spergel; Michael A. Strauss; Yuma Sugahara; Naoshi Sugiyama; Yasushi Suto; Nao Suzuki; Philip J. Tait; Masahiro Takada; Tsuyoshi Terai; Yoshiki Toba; Edwin L. Turner; Hisakazu Uchiyama; Keiichi Umetsu; Yuji Urata; Tomonori Usuda; Sherry Yeh; Suraphong Yuma

doi:10.1093/pasj/psx081

First data release of the Hyper Suprime-Cam Subaru Strategic Program

Hiroaki Aihara, Robert Armstrong, Steven Bickerton, James Bosch, Jean Coupon, Hisanori Furusawa, Yusuke Hayashi, Hiroyuki Ikeda, Yukiko Kamata, Hiroshi Karoji, Satoshi Kawanomoto, Michitaro Koike, Yutaka Komiyama, Dustin Lang, Robert H. Lupton, Sogo Mineo, Hironao Miyatake, Satoshi Miyazaki, Tomoki Morokuma, Yoshiyuki ObuchiYukie Oishi, Yuki Okura, Paul A. Price, Tadafumi Takata, Manobu M. Tanaka, Masayuki Tanaka, Yoko Tanaka, Tomohisa Uchida, Fumihiro Uraguchi, Yousuke Utsumi, Shiang Yu Wang, Yoshihiko Yamada, Hitomi Yamanoi, Naoki Yasuda, Nobuo Arimoto, Masashi Chiba, Francois Finet, Hiroki Fujimori, Seiji Fujimoto, Junko Furusawa, Tomotsugu Goto, Andy Goulding, James E. Gunn, Yuichi Harikane, Takashi Hattori, Masao Hayashi, Krzysztof G. Helminiak, Ryo Higuchi, Chiaki Hikage, Paul T.P. Ho, Bau Ching Hsieh, Kuiyun Huang, Song Huang, Masatoshi Imanishi, Ikuru Iwata, Anton T. Jaelani, Hung Yu Jian, Nobunari Kashikawa, Nobuhiko Katayama, Takashi Kojima, Akira Konno, Shintaro Koshida, Haruka Kusakabe, Alexie Leauthaud, Chien Hsiu Lee, Lihwai Lin, Yen Ting Lin, Rachel Mandelbaum, Yoshiki Matsuoka, Elinor Medezinski, Shoken Miyama, Rieko Momose, Anupreeta More, Surhud More, Shiro Mukae, Ryoma Murata, Hitoshi Murayama, Tohru Nagao, Fumiaki Nakata, Mana Niida, Hiroko Niikura, Atsushi J. Nishizawa, Masamune Oguri, Nobuhiro Okabe, Yoshiaki Ono, Masato Onodera, Masafusa Onoue, Masami Ouchi, Tae Soo Pyo, Takatoshi Shibuya, Kazuhiro Shimasaku, Melanie Simet, Joshua Speagle, David N. Spergel, Michael A. Strauss, Yuma Sugahara, Naoshi Sugiyama, Yasushi Suto, Nao Suzuki, Philip J. Tait, Masahiro Takada, Tsuyoshi Terai, Yoshiki Toba, Edwin L. Turner, Hisakazu Uchiyama, Keiichi Umetsu, Yuji Urata, Tomonori Usuda, Sherry Yeh, Suraphong Yuma

Research output: Contribution to journal › Article › peer-review

357 Scopus citations

Abstract

The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most important outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope, and it started in 2014 March. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7yr of observations (61.5 nights), and each of the Wide, Deep, and UltraDeep layers covers about 108, 26, and 4 square degrees down to depths of i ∼ 26.4, ∼26.5, and ∼27.0mag, respectively (5a for point sources). All the layers are observed in five broad bands (grizy), and the Deep and UltraDeep layers are observed in narrow bands as well. We achieve an impressive image quality of 0".6 in the i band in the Wide layer. We show that we achieve 1%-2% point spread function (PSF) photometry (root mean square) both internally and externally (against Pan-STARRS1), and ∼10mas and 40 mas internal and external astrometric accuracy, respectively. Both the calibrated images and catalogs are made available to the community through dedicated user interfaces and database servers. In addition to the pipeline products, we also provide value-added products such as photometric redshifts and a collection of public spectroscopic redshifts. Detailed descriptions of all the data can be found online.

Original language	English (US)
Article number	S8
Journal	Publications of the Astronomical Society of Japan
Volume	70
Issue number	Special Issue 1
DOIs	https://doi.org/10.1093/pasj/psx081
State	Published - Jan 2018

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Astronomical databases
Cosmology: observations
Galaxies: general
Surveys

Access to Document

10.1093/pasj/psx081

Cite this

Aihara, H., Armstrong, R., Bickerton, S., Bosch, J., Coupon, J., Furusawa, H., Hayashi, Y., Ikeda, H., Kamata, Y., Karoji, H., Kawanomoto, S., Koike, M., Komiyama, Y., Lang, D., Lupton, R. H., Mineo, S., Miyatake, H., Miyazaki, S., Morokuma, T., ... Yuma, S. (2018). First data release of the Hyper Suprime-Cam Subaru Strategic Program. Publications of the Astronomical Society of Japan, 70(Special Issue 1), [S8]. https://doi.org/10.1093/pasj/psx081

@article{41df784fcdb548c5a0026902d8f85104,

title = "First data release of the Hyper Suprime-Cam Subaru Strategic Program",

abstract = "The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most important outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope, and it started in 2014 March. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7yr of observations (61.5 nights), and each of the Wide, Deep, and UltraDeep layers covers about 108, 26, and 4 square degrees down to depths of i ∼ 26.4, ∼26.5, and ∼27.0mag, respectively (5a for point sources). All the layers are observed in five broad bands (grizy), and the Deep and UltraDeep layers are observed in narrow bands as well. We achieve an impressive image quality of 0{"}.6 in the i band in the Wide layer. We show that we achieve 1%-2% point spread function (PSF) photometry (root mean square) both internally and externally (against Pan-STARRS1), and ∼10mas and 40 mas internal and external astrometric accuracy, respectively. Both the calibrated images and catalogs are made available to the community through dedicated user interfaces and database servers. In addition to the pipeline products, we also provide value-added products such as photometric redshifts and a collection of public spectroscopic redshifts. Detailed descriptions of all the data can be found online.",

keywords = "Astronomical databases, Cosmology: observations, Galaxies: general, Surveys",

author = "Hiroaki Aihara and Robert Armstrong and Steven Bickerton and James Bosch and Jean Coupon and Hisanori Furusawa and Yusuke Hayashi and Hiroyuki Ikeda and Yukiko Kamata and Hiroshi Karoji and Satoshi Kawanomoto and Michitaro Koike and Yutaka Komiyama and Dustin Lang and Lupton, {Robert H.} and Sogo Mineo and Hironao Miyatake and Satoshi Miyazaki and Tomoki Morokuma and Yoshiyuki Obuchi and Yukie Oishi and Yuki Okura and Price, {Paul A.} and Tadafumi Takata and Tanaka, {Manobu M.} and Masayuki Tanaka and Yoko Tanaka and Tomohisa Uchida and Fumihiro Uraguchi and Yousuke Utsumi and Wang, {Shiang Yu} and Yoshihiko Yamada and Hitomi Yamanoi and Naoki Yasuda and Nobuo Arimoto and Masashi Chiba and Francois Finet and Hiroki Fujimori and Seiji Fujimoto and Junko Furusawa and Tomotsugu Goto and Andy Goulding and Gunn, {James E.} and Yuichi Harikane and Takashi Hattori and Masao Hayashi and Helminiak, {Krzysztof G.} and Ryo Higuchi and Chiaki Hikage and Ho, {Paul T.P.} and Hsieh, {Bau Ching} and Kuiyun Huang and Song Huang and Masatoshi Imanishi and Ikuru Iwata and Jaelani, {Anton T.} and Jian, {Hung Yu} and Nobunari Kashikawa and Nobuhiko Katayama and Takashi Kojima and Akira Konno and Shintaro Koshida and Haruka Kusakabe and Alexie Leauthaud and Lee, {Chien Hsiu} and Lihwai Lin and Lin, {Yen Ting} and Rachel Mandelbaum and Yoshiki Matsuoka and Elinor Medezinski and Shoken Miyama and Rieko Momose and Anupreeta More and Surhud More and Shiro Mukae and Ryoma Murata and Hitoshi Murayama and Tohru Nagao and Fumiaki Nakata and Mana Niida and Hiroko Niikura and Nishizawa, {Atsushi J.} and Masamune Oguri and Nobuhiro Okabe and Yoshiaki Ono and Masato Onodera and Masafusa Onoue and Masami Ouchi and Pyo, {Tae Soo} and Takatoshi Shibuya and Kazuhiro Shimasaku and Melanie Simet and Joshua Speagle and Spergel, {David N.} and Strauss, {Michael A.} and Yuma Sugahara and Naoshi Sugiyama and Yasushi Suto and Nao Suzuki and Tait, {Philip J.} and Masahiro Takada and Tsuyoshi Terai and Yoshiki Toba and Turner, {Edwin L.} and Hisakazu Uchiyama and Keiichi Umetsu and Yuji Urata and Tomonori Usuda and Sherry Yeh and Suraphong Yuma",

note = "Funding Information: the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. 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. GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalog is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT, and ASKAP, providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. Funding for the DEEP2 Galaxy Redshift Survey has been provided by NSF grants AST-95-09298, AST-0071048, AST-0507428, and AST-0507483, as well as NASA LTSA grant NNG04GC89G. Funding for PRIMUS is provided by NSF (AST-0607701, AST-0908246, AST-0908442, AST-0908354) and NASA (Spitzer-1356708, 08-ADP08-0019, NNX09AC95G). HM is supported by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work is in part supported by MEXT Grant-in-Aid for Scientific Research on Innovative Areas (Nos. 15H05887, 15H05892, 15H05893). Funding Information: This work is also based on zCOSMOS observations carried out using the Very Large Telescope at the ESO Paranal Observatory under Program ID: LP175.A-0839, on observations taken by the 3D-HST Treasury Program (GO 12177 and 12328) with the NASA/ESA HST, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555, on data from the VIMOS VLT Deep Survey, obtained from the VVDS database operated by Cesam, Laboratoire d{\textquoteright}Astrophysique de Marseille, France, on data from the VIMOS Public Extragalactic Redshift Survey (VIPERS). VIPERS has been performed using the ESO Very Large Telescope, under Large Program 182.A-0886. The participating institutions and funding agencies are listed at http://vipers.inaf.it. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, Funding Information: The Pan-STARRS1 Surveys 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, Eotvos Lorand University (ELTE), and the Los Alamos National Laboratory. Funding Information: 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 the Japanese Cabinet Office, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), the Japan Science and Technology Agency (JST), the Toray Science Foundation, NAOJ, Kavli IPMU, KEK, ASIAA, and Princeton University. Funding Information: 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 the Japanese Cabinet Office, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), the 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 http://dm.lsst.org. The Pan-STARRS1 Surveys 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'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, Eotvos Lorand University (ELTE), and the Los Alamos National Laboratory. This paper is based on data collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by the Subaru Telescope and Astronomy Data Center at the National Astronomical Observatory of Japan. We thank the anonymous referee for a useful report, which helped to improve the paper. This work is also based on zCOSMOS observations carried out using the Very Large Telescope at the ESO Paranal Observatory under Program ID: LP175.A-0839, on observations taken by the 3D-HST Treasury Program (GO 12177 and 12328) with the NASA/ESA HST, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555, on data from the VIMOS VLT Deep Survey, obtained from the VVDS database operated by Cesam, Laboratoire d'Astrophysique de Marseille, France, on data from the VIMOS Public Extragalactic Redshift Survey (VIPERS). VIPERS has been performed using the ESO Very Large Telescope, under Large Program 182.A-0886. The participating institutions and funding agencies are listed at http://vipers.inaf.it. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. 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. GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalog is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT, and ASKAP, providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. Funding for the DEEP2 Galaxy Redshift Survey has been provided by NSF grants AST-95-09298, AST-0071048, AST-0507428, and AST-0507483, aswell asNASALTSA grant NNG04GC89G. Funding for PRIMUS is provided by NSF (AST-0607701, AST-0908246, AST-0908442, AST-0908354) and NASA (Spitzer-1356708, 08-ADP08-0019, NNX09AC95G). HM is supported by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work is in part supported by MEXT Grant-in-Aid for Scientific Research on Innovative Areas (Nos. 15H05887, 15H05892, 15H05893). Publisher Copyright: {\textcopyright} The Author 2017. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved.",

year = "2018",

month = jan,

doi = "10.1093/pasj/psx081",

language = "English (US)",

volume = "70",

journal = "Publication of the Astronomical Society of Japan",

issn = "0004-6264",

publisher = "Astronomical Society of Japan",

number = "Special Issue 1",

}

Aihara, H, Armstrong, R, Bickerton, S, Bosch, J, Coupon, J, Furusawa, H, Hayashi, Y, Ikeda, H, Kamata, Y, Karoji, H, Kawanomoto, S, Koike, M, Komiyama, Y, Lang, D, Lupton, RH, Mineo, S, Miyatake, H, Miyazaki, S, Morokuma, T, Obuchi, Y, Oishi, Y, Okura, Y, Price, PA, Takata, T, Tanaka, MM, Tanaka, M, Tanaka, Y, Uchida, T, Uraguchi, F, Utsumi, Y, Wang, SY, Yamada, Y, Yamanoi, H, Yasuda, N, Arimoto, N, Chiba, M, Finet, F, Fujimori, H, Fujimoto, S, Furusawa, J, Goto, T, Goulding, A, Gunn, JE, Harikane, Y, Hattori, T, Hayashi, M, Helminiak, KG, Higuchi, R, Hikage, C, Ho, PTP, Hsieh, BC, Huang, K, Huang, S, Imanishi, M, Iwata, I, Jaelani, AT, Jian, HY, Kashikawa, N, Katayama, N, Kojima, T, Konno, A, Koshida, S, Kusakabe, H, Leauthaud, A, Lee, CH, Lin, L, Lin, YT, Mandelbaum, R, Matsuoka, Y, Medezinski, E, Miyama, S, Momose, R, More, A, More, S, Mukae, S, Murata, R, Murayama, H, Nagao, T, Nakata, F, Niida, M, Niikura, H, Nishizawa, AJ, Oguri, M, Okabe, N, Ono, Y, Onodera, M, Onoue, M, Ouchi, M, Pyo, TS, Shibuya, T, Shimasaku, K, Simet, M, Speagle, J, Spergel, DN, Strauss, MA, Sugahara, Y, Sugiyama, N, Suto, Y, Suzuki, N, Tait, PJ, Takada, M, Terai, T, Toba, Y, Turner, EL, Uchiyama, H, Umetsu, K, Urata, Y, Usuda, T, Yeh, S & Yuma, S 2018, 'First data release of the Hyper Suprime-Cam Subaru Strategic Program', Publications of the Astronomical Society of Japan, vol. 70, no. Special Issue 1, S8. https://doi.org/10.1093/pasj/psx081

TY - JOUR

T1 - First data release of the Hyper Suprime-Cam Subaru Strategic Program

AU - Aihara, Hiroaki

AU - Armstrong, Robert

AU - Bickerton, Steven

AU - Bosch, James

AU - Coupon, Jean

AU - Furusawa, Hisanori

AU - Hayashi, Yusuke

AU - Ikeda, Hiroyuki

AU - Kamata, Yukiko

AU - Karoji, Hiroshi

AU - Kawanomoto, Satoshi

AU - Koike, Michitaro

AU - Komiyama, Yutaka

AU - Lang, Dustin

AU - Lupton, Robert H.

AU - Mineo, Sogo

AU - Miyatake, Hironao

AU - Miyazaki, Satoshi

AU - Morokuma, Tomoki

AU - Obuchi, Yoshiyuki

AU - Oishi, Yukie

AU - Okura, Yuki

AU - Price, Paul A.

AU - Takata, Tadafumi

AU - Tanaka, Manobu M.

AU - Tanaka, Masayuki

AU - Tanaka, Yoko

AU - Uchida, Tomohisa

AU - Uraguchi, Fumihiro

AU - Utsumi, Yousuke

AU - Wang, Shiang Yu

AU - Yamada, Yoshihiko

AU - Yamanoi, Hitomi

AU - Yasuda, Naoki

AU - Arimoto, Nobuo

AU - Chiba, Masashi

AU - Finet, Francois

AU - Fujimori, Hiroki

AU - Fujimoto, Seiji

AU - Furusawa, Junko

AU - Goto, Tomotsugu

AU - Goulding, Andy

AU - Gunn, James E.

AU - Harikane, Yuichi

AU - Hattori, Takashi

AU - Hayashi, Masao

AU - Helminiak, Krzysztof G.

AU - Higuchi, Ryo

AU - Hikage, Chiaki

AU - Ho, Paul T.P.

AU - Hsieh, Bau Ching

AU - Huang, Kuiyun

AU - Huang, Song

AU - Imanishi, Masatoshi

AU - Iwata, Ikuru

AU - Jaelani, Anton T.

AU - Jian, Hung Yu

AU - Kashikawa, Nobunari

AU - Katayama, Nobuhiko

AU - Kojima, Takashi

AU - Konno, Akira

AU - Koshida, Shintaro

AU - Kusakabe, Haruka

AU - Leauthaud, Alexie

AU - Lee, Chien Hsiu

AU - Lin, Lihwai

AU - Lin, Yen Ting

AU - Mandelbaum, Rachel

AU - Matsuoka, Yoshiki

AU - Medezinski, Elinor

AU - Miyama, Shoken

AU - Momose, Rieko

AU - More, Anupreeta

AU - More, Surhud

AU - Mukae, Shiro

AU - Murata, Ryoma

AU - Murayama, Hitoshi

AU - Nagao, Tohru

AU - Nakata, Fumiaki

AU - Niida, Mana

AU - Niikura, Hiroko

AU - Nishizawa, Atsushi J.

AU - Oguri, Masamune

AU - Okabe, Nobuhiro

AU - Ono, Yoshiaki

AU - Onodera, Masato

AU - Onoue, Masafusa

AU - Ouchi, Masami

AU - Pyo, Tae Soo

AU - Shibuya, Takatoshi

AU - Shimasaku, Kazuhiro

AU - Simet, Melanie

AU - Speagle, Joshua

AU - Spergel, David N.

AU - Strauss, Michael A.

AU - Sugahara, Yuma

AU - Sugiyama, Naoshi

AU - Suto, Yasushi

AU - Suzuki, Nao

AU - Tait, Philip J.

AU - Takada, Masahiro

AU - Terai, Tsuyoshi

AU - Toba, Yoshiki

AU - Turner, Edwin L.

AU - Uchiyama, Hisakazu

AU - Umetsu, Keiichi

AU - Urata, Yuji

AU - Usuda, Tomonori

AU - Yeh, Sherry

AU - Yuma, Suraphong

N1 - Funding Information: the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. 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. GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalog is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT, and ASKAP, providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. Funding for the DEEP2 Galaxy Redshift Survey has been provided by NSF grants AST-95-09298, AST-0071048, AST-0507428, and AST-0507483, as well as NASA LTSA grant NNG04GC89G. Funding for PRIMUS is provided by NSF (AST-0607701, AST-0908246, AST-0908442, AST-0908354) and NASA (Spitzer-1356708, 08-ADP08-0019, NNX09AC95G). HM is supported by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work is in part supported by MEXT Grant-in-Aid for Scientific Research on Innovative Areas (Nos. 15H05887, 15H05892, 15H05893). Funding Information: This work is also based on zCOSMOS observations carried out using the Very Large Telescope at the ESO Paranal Observatory under Program ID: LP175.A-0839, on observations taken by the 3D-HST Treasury Program (GO 12177 and 12328) with the NASA/ESA HST, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555, on data from the VIMOS VLT Deep Survey, obtained from the VVDS database operated by Cesam, Laboratoire d’Astrophysique de Marseille, France, on data from the VIMOS Public Extragalactic Redshift Survey (VIPERS). VIPERS has been performed using the ESO Very Large Telescope, under Large Program 182.A-0886. The participating institutions and funding agencies are listed at http://vipers.inaf.it. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, Funding Information: The Pan-STARRS1 Surveys 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’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, Eotvos Lorand University (ELTE), and the Los Alamos National Laboratory. Funding Information: 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 the Japanese Cabinet Office, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), the Japan Science and Technology Agency (JST), the Toray Science Foundation, NAOJ, Kavli IPMU, KEK, ASIAA, and Princeton University. Funding Information: 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 the Japanese Cabinet Office, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), the 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 http://dm.lsst.org. The Pan-STARRS1 Surveys 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'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, Eotvos Lorand University (ELTE), and the Los Alamos National Laboratory. This paper is based on data collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by the Subaru Telescope and Astronomy Data Center at the National Astronomical Observatory of Japan. We thank the anonymous referee for a useful report, which helped to improve the paper. This work is also based on zCOSMOS observations carried out using the Very Large Telescope at the ESO Paranal Observatory under Program ID: LP175.A-0839, on observations taken by the 3D-HST Treasury Program (GO 12177 and 12328) with the NASA/ESA HST, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555, on data from the VIMOS VLT Deep Survey, obtained from the VVDS database operated by Cesam, Laboratoire d'Astrophysique de Marseille, France, on data from the VIMOS Public Extragalactic Redshift Survey (VIPERS). VIPERS has been performed using the ESO Very Large Telescope, under Large Program 182.A-0886. The participating institutions and funding agencies are listed at http://vipers.inaf.it. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. 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. GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalog is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT, and ASKAP, providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. Funding for the DEEP2 Galaxy Redshift Survey has been provided by NSF grants AST-95-09298, AST-0071048, AST-0507428, and AST-0507483, aswell asNASALTSA grant NNG04GC89G. Funding for PRIMUS is provided by NSF (AST-0607701, AST-0908246, AST-0908442, AST-0908354) and NASA (Spitzer-1356708, 08-ADP08-0019, NNX09AC95G). HM is supported by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work is in part supported by MEXT Grant-in-Aid for Scientific Research on Innovative Areas (Nos. 15H05887, 15H05892, 15H05893). Publisher Copyright: © The Author 2017. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved.

PY - 2018/1

Y1 - 2018/1

N2 - The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most important outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope, and it started in 2014 March. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7yr of observations (61.5 nights), and each of the Wide, Deep, and UltraDeep layers covers about 108, 26, and 4 square degrees down to depths of i ∼ 26.4, ∼26.5, and ∼27.0mag, respectively (5a for point sources). All the layers are observed in five broad bands (grizy), and the Deep and UltraDeep layers are observed in narrow bands as well. We achieve an impressive image quality of 0".6 in the i band in the Wide layer. We show that we achieve 1%-2% point spread function (PSF) photometry (root mean square) both internally and externally (against Pan-STARRS1), and ∼10mas and 40 mas internal and external astrometric accuracy, respectively. Both the calibrated images and catalogs are made available to the community through dedicated user interfaces and database servers. In addition to the pipeline products, we also provide value-added products such as photometric redshifts and a collection of public spectroscopic redshifts. Detailed descriptions of all the data can be found online.

AB - The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most important outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope, and it started in 2014 March. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7yr of observations (61.5 nights), and each of the Wide, Deep, and UltraDeep layers covers about 108, 26, and 4 square degrees down to depths of i ∼ 26.4, ∼26.5, and ∼27.0mag, respectively (5a for point sources). All the layers are observed in five broad bands (grizy), and the Deep and UltraDeep layers are observed in narrow bands as well. We achieve an impressive image quality of 0".6 in the i band in the Wide layer. We show that we achieve 1%-2% point spread function (PSF) photometry (root mean square) both internally and externally (against Pan-STARRS1), and ∼10mas and 40 mas internal and external astrometric accuracy, respectively. Both the calibrated images and catalogs are made available to the community through dedicated user interfaces and database servers. In addition to the pipeline products, we also provide value-added products such as photometric redshifts and a collection of public spectroscopic redshifts. Detailed descriptions of all the data can be found online.

KW - Astronomical databases

KW - Cosmology: observations

KW - Galaxies: general

KW - Surveys

UR - http://www.scopus.com/inward/record.url?scp=85041210432&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85041210432&partnerID=8YFLogxK

U2 - 10.1093/pasj/psx081

DO - 10.1093/pasj/psx081

M3 - Article

AN - SCOPUS:85041210432

SN - 0004-6264

VL - 70

JO - Publication of the Astronomical Society of Japan

JF - Publication of the Astronomical Society of Japan

IS - Special Issue 1

M1 - S8

ER -

First data release of the Hyper Suprime-Cam Subaru Strategic Program

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