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Near-Infrared Imaging with the 105 cm Kiso Schmidt

Published online by Cambridge University Press:  12 April 2016

T. Ichikawa ,
K. Tarusawa ,
K. Yanagisawa  and
N. Itoh
T. Ichikawa
Affiliation:
Kiso Observatory, The University of Tokyo, Mitake-mura, Kiso-gun, Nagano 397-01, Japan
K. Tarusawa
Affiliation:
Kiso Observatory, The University of Tokyo, Mitake-mura, Kiso-gun, Nagano 397-01, Japan
K. Yanagisawa
Affiliation:
Department of Astronomy, The University of Tokyo, Yayoi, Bunkyo-ku, Tokyo 113, Japan
N. Itoh
Affiliation:
Department of Astronomy, The University of Tokyo, Yayoi, Bunkyo-ku, Tokyo 113, Japan

Abstract

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We have carried out imaging observations in the near-infrared (J, H and K’ band) with a large format array camera attached to the prime focus of the 105 cm Schmidt telescope at Kiso Observatory. The image resolution, limiting magnitudes and effect of thermal radiation are presented, based on observations of nearby galaxies. Considering the results, we are constructing a new larger near-infrared camera optimized for use with the Kiso Schmidt.

Type
III. The Use of CCDs in Schmidt Telescopes
Information
International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 48 - 51
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

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