Hyper Suprime-Cam: characteristics of 116 fully depleted back-illuminated CCDs

Yukiko Kamata; Satoshi Miyazaki; Hidehiko Nakaya; Yutaka Komiyama; Yoshiyuki Obuchi; Satoshi Kawanomoto; Fumihiro Uraguchi; Yosuke Utsumi; Hisanori Suzuki; Yasuhito Miyazaki; Masaharu Muramatsu

doi:10.1117/12.927234

25 September 2012 Hyper Suprime-Cam: characteristics of 116 fully depleted back-illuminated CCDs

Yukiko Kamata, Satoshi Miyazaki, Hidehiko Nakaya, Yutaka Komiyama, Yoshiyuki Obuchi, Satoshi Kawanomoto, Fumihiro Uraguchi, Yosuke Utsumi, Hisanori Suzuki, Yasuhito Miyazaki, Masaharu Muramatsu

Author Affiliations +

Proceedings Volume 8453, High Energy, Optical, and Infrared Detectors for Astronomy V; 84531X (2012) https://doi.org/10.1117/12.927234
Event: SPIE Astronomical Telescopes + Instrumentation, 2012, Amsterdam, Netherlands

Abstract

Hyper Suprime-Cam (HSC)¹,² is a wide field imaging camera with the field of view (FOV) 1.5 degree diameter, which is to be installed at the prime focus of the Subaru Telescope. The large FOV is realized by the 116 2K × 4K pixels fully depleted back-illuminated CCD (FDCCD) with 15 μm pixel square. The acceptance inspection of the CCDs started around the end of 2009 and finished June 2011. We measured basic characteristics such as charge transfer efficiency (CTE), dark current, readout noise, linearity and the number of the dead column for all CCDs, and measured the quantum effciency (QE) of 21 CCDs. As a result, we confirmed exceptional quality and performance fdor all CCDs ans were able to select the best pissible 116 CCDs. We also measured the flatness of each CCD at room temperature, and optimally placed them on the focal plane plate. In this paper, we report the results of the acceptance inspection asn the installation process into the HSC dewar³,⁴.

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Yukiko Kamata, Satoshi Miyazaki, Hidehiko Nakaya, Yutaka Komiyama, Yoshiyuki Obuchi, Satoshi Kawanomoto, Fumihiro Uraguchi, Yosuke Utsumi, Hisanori Suzuki, Yasuhito Miyazaki, and Masaharu Muramatsu "Hyper Suprime-Cam: characteristics of 116 fully depleted back-illuminated CCDs", Proc. SPIE 8453, High Energy, Optical, and Infrared Detectors for Astronomy V, 84531X (25 September 2012); https://doi.org/10.1117/12.927234

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