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

被引：524

作者：

Aihara, Hiroaki ^{[1
]}

Armstrong, Robert ^{[2
]}

Bickerton, Steven ^{[3
]}

Bosch, James ^{[2
]}

Coupon, Jean ^{[4
]}

Furusawa, Hisanori ^{[5
]}

Hayashi, Yusuke ^{[5
]}

Ikeda, Hiroyuki ^{[5
]}

Kamata, Yukiko ^{[5
]}

Karoji, Hiroshi ^{[2
,6
]}

Kawanomoto, Satoshi ^{[5
]}

Koike, Michitaro ^{[5
]}

Komiyama, Yutaka ^{[5
,7
]}

Lang, Dustin ^{[8
,9
]}

Lupton, Robert H. ^{[2
]}

Mineo, Sogo ^{[5
]}

Miyatake, Hironao ^{[10
,11
]}

Miyazaki, Satoshi ^{[5
,7
]}

Morokuma, Tomoki ^{[11
,12
]}

Obuchi, Yoshiyuki ^{[5
]}

Oishi, Yukie ^{[5
]}

Okura, Yuki ^{[13
,14
]}

Price, Paul A. ^{[2
]}

Takata, Tadafumi ^{[5
,7
]}

Tanaka, Manobu M. ^{[15
]}

Tanaka, Masayuki ^{[5
]}

Tanaka, Yoko ^{[16
]}

Uchida, Tomohisa ^{[15
]}

Uraguchi, Fumihiro ^{[5
]}

Utsumi, Yousuke ^{[17
]}

Wang, Shiang-Yu ^{[18
]}

Yamada, Yoshihiko ^{[5
]}

Yamanoi, Hitomi ^{[5
]}

Yasuda, Naoki ^{[11
]}

Arimoto, Nobuo ^{[7
,16
]}

Chiba, Masashi ^{[19
]}

Finet, Francois ^{[16
]}

Fujimori, Hiroki ^{[20
]}

Fujimoto, Seiji ^{[21
]}

Furusawa, Junko ^{[5
]}

Goto, Tomotsugu ^{[22
]}

Goulding, Andy ^{[2
]}

Gunn, James E. ^{[2
]}

Harikane, Yuichi ^{[1
,21
]}

Hattori, Takashi ^{[16
]}

Hayashi, Masao ^{[5
]}

Helminiak, Krzysztof G. ^{[23
]}

Higuchi, Ryo ^{[1
,21
]}

Hikage, Chiaki ^{[11
]}

Ho, Paul T. P. ^{[18
,24
]}

机构：

[1] Univ Tokyo, Dept Phys, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[2] Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA

[3] Orbital Insight, 100 W Evelyn Ave, Mountain View, CA 94041 USA

[4] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[5] Natl Astron Observ, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[6] Natl Inst Nat Sci, Minato Ku, 4-3-13 Toranomon, Tokyo 1050001, Japan

[7] Grad Univ Adv Studies SOKENDAI, Sch Sci, Dept Astron, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[8] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada

[9] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada

[10] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[11] Univ Tokyo, Kavli Inst Phys & Math Univ Kavli IPMU WPI, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan

[12] Univ Tokyo, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan

[13] RIKEN High Energy Astrophys Lab, 2-1 Hirosawa, Wako, Saitama 3510198, Japan

[14] Brookhaven Natl Lab, RIKEN BNL Res Ctr, Bldg 510A,20 Penn St, Upton, NY 11973 USA

[15] High Energy Accelerator Res Org, Inst Particle & Nucl Studies, 203-1 Shirakata, Tokai, Ibaraki 3191106, Japan

[16] Natl Astron Observ Japan, Subaru Telescope, 650 N Aohoku Pl, Hilo, HI 96720 USA

[17] Hiroshima Univ, Hiroshima Astrophys Sci Ctr, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan

[18] Acad Sinica, Inst Astron & Astrophys, POB 23-141, Taipei 10617, Taiwan

[19] Tohoku Univ, Astron Inst, Aoba Ku, 6-3 Aramaki, Sendai, Miyagi 9808578, Japan

[20] Meisei Elect Co Ltd, 2223 Naganuma, Naganuma, Gunma 3728585, Japan

[21] Univ Tokyo, Inst Cosm Ray Res, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778582, Japan

[22] Natl Tsing Hua Univ, Inst Astron, 101 Sect 2 Kuang Fu Rd, Hsinchu 30013, Taiwan

[23] Nicolaus Copernicus Astron Ctr, Dept Astrophys, Ul Rabianska 8, PL-87100 Torun, Poland

[24] East Asian Observ, 660 N Aohoku Pl,Univ Pk, Hilo, HI 96720 USA

[25] Natl Taiwan Normal Univ, Dept Math Sci, New Taipei 24449, Taiwan

[26] Univ Calif Santa Cruz, Dept Astron & Astrophys, 1156 High St, Santa Cruz, CA 95064 USA

[27] Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[28] Carnegie Mellon Univ, Dept Phys, McWilliams Ctr Cosmol, Pittsburgh, PA 15213 USA

[29] Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan

[30] Kobe Univ, Integrated Res Ctr, Ctr Planetary Sci, Chuo Ku, 7-1-48 Minamimachi, Kobe, Hyogo 6500047, Japan

[31] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[32] Univ Calif Berkeley, Ctr Japanese Studies, Berkeley, CA 94720 USA

[33] Lawrence Berkeley Natl Lab, Theoret Phys Grp, MS 50A 5104, Berkeley, CA 94720 USA

[34] Ehime Univ, Grad Sch Sci & Engn, Bunkyo Cho 2-5, Matsuyama, Ehime 7908577, Japan

[35] Nagoya Univ, Institute Adv Res, Chikusa Ku, Nagoya, Aichi 4648602, Japan

[36] Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, Tokyo 1130033, Japan

[37] Hiroshima Univ, Dept Phys Sci, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan

[38] Univ Calif Riverside, 900 Univ Ave, Riverside, CA 92521 USA

[39] Harvard Univ, 60 Garden St, Cambridge, MA 02138 USA

[40] Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA

[41] Nagoya Univ, Dept Phys & Astrophys, Chikusa Ku, Nagoya, Aichi 4648602, Japan

[42] Natl Cent Univ, Inst Astron, Chungli 32054, Taiwan

[43] Mahidol Univ, Dept Phys, Fac Sci, Bangkok 10400, Thailand

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2018年 / 70卷

基金：

美国国家科学基金会; 美国国家航空航天局; 日本学术振兴会; 日本科学技术振兴机构;

关键词：

astronomical databases; cosmology: observations; galaxies: general; surveys; DARK ENERGY SURVEY; CATALOG; COSMOS; GALAXY; PHOTOMETRY; EVOLUTION;

D O I：

10.1093/pasj/psx081

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 1.7 yr 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 similar to 26.4, similar to 26.5, and similar to 27.0 mag, respectively (5 sigma 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 similar to 10 mas 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 spectro-scopic redshifts. Detailed descriptions of all the data can be found online. The data release website is https://hsc-release.mtk.nao.ac.jp.

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