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Near-Infrared Imaging by a Schmidt Telescope

Published online by Cambridge University Press:  26 July 2016

K. Yanagisawa ,
N. Itoh ,
T. Ichikawa ,
K. Tarusawa  and
M. Ueno
K. Yanagisawa
Affiliation:
Department of Astronomy, University of Tokyo, Yayoi, Bunkyo-ku, Tokyo 113, Japan
N. Itoh
Affiliation:
Department of Astronomy, University of Tokyo, Yayoi, Bunkyo-ku, Tokyo 113, Japan
T. Ichikawa
Affiliation:
Kiso Observatory, University of Tokyo, Mitake-Mura, Kiso-gun, Nagano 397-01, Japan
K. Tarusawa
Affiliation:
Kiso Observatory, University of Tokyo, Mitake-Mura, Kiso-gun, Nagano 397-01, Japan
M. Ueno
Affiliation:
College of Arts and Science, University of Tokyo, Komaba, Meguro-ku, Tokyo 253, Japan

Abstract

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We have carried out wide field 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 the effect of thermal radiation are discussed.

Type
Part Two: Digital Detectors in Wide-Field Imaging
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 89 - 90
Copyright
Copyright © Kluwer 1994 

References

Kimata, M. et al., 1987. IEEE Journal of Solid State Circuits, sc-22 6, 1124.Google Scholar
Ueno, M. et al., 1992. S.P.I.E., 1762, 423.Google Scholar