# 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, 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, C.-H. 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, 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, and Suraphong Yuma

arXiv: 1702.08449 · 2018-02-14

## TL;DR

The first public data release of the Hyper Suprime-Cam Subaru Strategic Program provides extensive imaging data across multiple layers and bands, with high image quality and precise photometry and astrometry, supporting astronomical research on dark matter and energy.

## Contribution

This paper presents the initial public data release of the HSC-SSP, including detailed imaging data, calibration, and value-added products, enabling broad community access and scientific analysis.

## Key findings

- Achieved 0.6 arcsec image quality in the i-band for the Wide layer.
- Achieved 1-2% photometric accuracy internally and against Pan-STARRS1.
- Achieved ~10 mas and 40 mas internal and external astrometric accuracy.

## Abstract

The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most 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 March 2014. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7 years 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 ~27.0 mag, respectively (5sigma 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 arcsec in the i-band in the Wide layer. We show that we achieve 1-2 per cent PSF photometry (rms) both internally and externally (against Pan-STARRS1), and ~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 spectroscopic redshifts. Detailed descriptions of all the data can be found online. The data release website is https://hsc-release.mtk.nao.ac.jp/.

## Full text

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## Figures

43 figures with captions in the complete paper: https://tomesphere.com/paper/1702.08449/full.md

## References

63 references — full list in the complete paper: https://tomesphere.com/paper/1702.08449/full.md

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Source: https://tomesphere.com/paper/1702.08449