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Proceedings Paper

First Paschen alpha imaging from the ground: the first light of Atacama Near-Infrared Camera on the miniTAO 1m telescope
Author(s): Kentaro Motohara; Masahiro Konishi; Koji Toshikawa; Natsuko Mitani; Shigeyuki Sako; Yuka K. Uchimoto; Tomoyasu Yamamuro; Takeo Minezaki; Toshihiko Tanabe; Takashi Miyata; Shintaro Koshida; Daisuke Kato; Ryo Ohsawa; Tomohiko Nakamura; Kentaro Asano; Yuzuru Yoshii; Mamoru Doi; Kotaro Kohno; Masuo Tanaka; Kimiaki Kawara; Toshihiro Handa; Tsutomu Aoki; Takao Soyano; Ken'ichi Tarusawa; Yoshifusa Ita
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Paper Abstract

We have developed a near infrared camera called ANIR (Atacama Near InfraRed camera) for the University of Tokyo Atacama 1.0m telescope installed at the summit of Co. Chajnantor (5640m altitude) in northern Chile. The camera is based on a PACE HAWAII-2 array with an Offner relay optics for re-imaging, and field of view is 5. 3 × 5. 3 with pixel scale of 0. 31/pix. It is also capable of optical/infrared simultaneous imaging by inserting a dichroic mirror before the focal plane. The high altitude and extremely low water vapor (PWV=0.5mm) of the site enables us to perform observation of hydrogen Paschenα (Paα) emission line at 1.8751 μm. The first light observation was carried out in July 2009, and we have successfully obtained Paα images of the Galactic center using the N1875 narrow-band filter. This is the first success of Paα imaging of a Galactic object from a ground based telescope. System efficiencies for the broad-band filters are measured to be 15% at the J-band and 30% at Ks, while that of the N1875 narrow-band filter, corresponding to Paα; wavelength, varies from 8 to 15%, which may be caused by fluctuation of the atmospheric transmittance. ATRAN simulation suggests that this corresponds to PWV of 0.3 - 1.5mm, consistent with previous results of the site testing. Measured seeing size is median ~0. 8, corresponding to the real seeing value of 0. 6 - 0. 8. These results demonstrates the excellent capability of the site for infrared observations.

Paper Details

Date Published: 20 July 2010
PDF: 10 pages
Proc. SPIE 7735, Ground-based and Airborne Instrumentation for Astronomy III, 77353K (20 July 2010); doi: 10.1117/12.856102
Show Author Affiliations
Kentaro Motohara, Institute of Astronomy, The Univ. of Tokyo (Japan)
Masahiro Konishi, Institute of Astronomy, The Univ. of Tokyo (Japan)
Koji Toshikawa, Institute of Astronomy, The Univ. of Tokyo (Japan)
Natsuko Mitani, Institute of Astronomy, The Univ. of Tokyo (Japan)
Shigeyuki Sako, Institute of Astronomy, The Univ. of Tokyo (Japan)
Yuka K. Uchimoto, Institute of Astronomy, The Univ. of Tokyo (Japan)
Tomoyasu Yamamuro, OptCraft (Japan)
Takeo Minezaki, Institute of Astronomy, The Univ. of Tokyo (Japan)
Toshihiko Tanabe, Institute of Astronomy, The Univ. of Tokyo (Japan)
Takashi Miyata, Institute of Astronomy, The Univ. of Tokyo (Japan)
Shintaro Koshida, Institute of Astronomy, The Univ. of Tokyo (Japan)
Daisuke Kato, The Univ. of Tokyo (Japan)
Institute of Space and Astronautical Science (Japan)
Ryo Ohsawa, The Univ. of Tokyo (Japan)
Tomohiko Nakamura, Institute of Astronomy, The Univ. of Tokyo (Japan)
Kentaro Asano, Institute of Astronomy, The Univ. of Tokyo (Japan)
Yuzuru Yoshii, Institute of Astronomy, The Univ. of Tokyo (Japan)
Mamoru Doi, Institute of Astronomy, The Univ. of Tokyo (Japan)
Kotaro Kohno, Institute of Astronomy, The Univ. of Tokyo (Japan)
Masuo Tanaka, Institute of Astronomy, The Univ. of Tokyo (Japan)
Kimiaki Kawara, Institute of Astronomy, The Univ. of Tokyo (Japan)
Toshihiro Handa, Institute of Astronomy, The Univ. of Tokyo (Japan)
Tsutomu Aoki, Kiso Observatory, The Univ. of Tokyo (Japan)
Takao Soyano, Kiso Observatory, The Univ. of Tokyo (Japan)
Ken'ichi Tarusawa, Kiso Observatory, The Univ. of Tokyo (Japan)
Yoshifusa Ita, National Astronomical Observatory of Japan (Japan)
Astronomical Institute, Tohoku Univ. (Japan)


Published in SPIE Proceedings Vol. 7735:
Ground-based and Airborne Instrumentation for Astronomy III
Ian S. McLean; Suzanne K. Ramsay; Hideki Takami, Editor(s)

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