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Please use this identifier to cite or link to this item: http://repository.li.mahidol.ac.th/dspace/handle/123456789/45753
Title: First data release of the Hyper Suprime-Cam Subaru Strategic Program
Authors: 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
High Energy Accelerator Research Organization, Institute of Particle and Nuclear Physics
Research Center for the Early Universe
Academia Sinica, Institute of Astronomy and Astrophysics
Hiroshima University
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
University of California, Riverside
Carnegie Mellon University
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
University of Tokyo
University of California, Berkeley
University of California, Santa Cruz
National Taiwan Normal University
The Graduate University for Advanced Studies
National Tsing Hua University
National Institutes of Natural Sciences
University of Toronto
Riken
Kobe University
Harvard University
Jet Propulsion Laboratory, California Institute of Technology
Tohoku University
Riken BNL Research Center
Lawrence Berkeley National Laboratory
Université de Genève
Princeton University
Ehime University
Nagoya University
Meisei Electric Co. Ltd.
Orbital Insight
Flatiron Institute
East Asian Observatory
Keywords: Earth and Planetary Sciences;Physics and Astronomy
Issue Date: 1-Jan-2018
Citation: Publications of the Astronomical Society of Japan. Vol.70, No.Special Issue 1 (2018)
Abstract: © The Author 2017. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved. 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.
URI: https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85041210432&origin=inward
http://repository.li.mahidol.ac.th/dspace/handle/123456789/45753
ISSN: 2053051X
00046264
Appears in Collections:Scopus 2018

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