Proc. SPIE, pp. 107020J

Authors:

  • Shigeyuki Sako
  • Ryou Ohsawa
  • Hidenori Takahashi
  • Yuto Kojima
  • Mamoru Doi
  • Naoto Kobayashi
  • Tsutomu Aoki
  • Noriaki Arima
  • Ko Arimatsu
  • Makoto Ichiki
  • Shiro Ikeda
  • Kota Inooka
  • Yoshifusa Ita
  • Toshihiro Kasuga
  • Mitsuru Kokubo
  • Masahiro Konishi
  • Hiroyuki Maehara
  • Noriyuki Matsunaga
  • Kazuma Mitsuda
  • Takashi Miyata
  • Yuki Mori
  • Mikio Morii
  • Tomoki Morokuma
  • Kentaro Motohara
  • Yoshikazu Nakada
  • Shin-Ichiro Okumura
  • Yuki Sarugaku
  • Mikiya Sato
  • Toshikazu Shigeyama
  • Takao Soyano
  • Masaomi Tanaka
  • Ken’ichi Tarusawa
  • Nozomu Tominaga
  • Tomonori Totani
  • Seitaro Urakawa
  • Fumihiko Usui
  • Junichi Watanabe
  • Takuya Yamashita
  • Makoto Yoshikawa

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Abstract:

The Tomo-e Gozen is a wide-field high-speed camera for the Kiso $1.0$ m Schmidt telescope, with a field-of-view of $20.7$ deg$^2$ covered by 84 chips of 2k$\times$1k CMOS image sensors with 19 ${\mu}$m pixels. It is capable to take consecutive images at 2 fps in full-frame read with an absolute time accuracy of 0.2 millisecond. The sensors are operated without mechanical coolers owing to a low dark current at room temperature. A low read noise of 2 e$^-$ achieves higher sensitivity than that with a CCD sensor in short exposures. Big data of 30 TBytes per night produced in the 2 fps observations is processed in real-time to quickly detect transient events and issue alerts for follow-ups.