9 August 2016 Okayama astrophysical observatory wide-field camera: status and performance
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Okayama Astrophysical Observatory Wide Field Camera is a near-infrared (0.9-2.5 μm) survey telescope, built as a renewal of 0.91 m classical Cassegrain telescope. The optics is composed of forward Cassegrain and quasi Schmidt, which yield an effective image circle of Φ51 mm. A HAWAII-1 PACE detector is placed at the focal plane, which gives a field of view of 0.48 deg.×0.48 deg. with image scale of 1.67 arcsec/pix. OAOWFC is used to monitor the Galactic plane for variability and search for EM counterpart of gravitational wave sources.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kenshi Yanagisawa, Kenshi Yanagisawa, Yasuhiro Shimizu, Yasuhiro Shimizu, Kiichi Okita, Kiichi Okita, Daisuke Kuroda, Daisuke Kuroda, Hironori Tsutsui, Hironori Tsutsui, Hiroyuki Toda, Hiroyuki Toda, Hideyuki Izumiura, Hideyuki Izumiura, Michitoshi Yoshida, Michitoshi Yoshida, Koji Ohta, Koji Ohta, Nobuyuki Kawai, Nobuyuki Kawai, "Okayama astrophysical observatory wide-field camera: status and performance", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99085D (9 August 2016); doi: 10.1117/12.2233745; https://doi.org/10.1117/12.2233745


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