Abstract
A 14-inch Schmidt plate contains 109 photographic grains and 105 to 106 images of stars and galaxies on it. Such a quantity of data is too large to be handled in a conventional way even for a big computer.
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References
Maehara, H. 1981, American Astron. Soc. Photo-Bulletin No. 26.
Maehara, H., and Watanabe, M. 1980, in “Optical and Infrared Telescopes for 1990’s”, (ed. A. Hewitt), p677.
Mizuno, S., Sakka, K., Sasaki, T., and Kogure, T. 1981, Astrophys. Space Sci. 78, 235.
Stobie, R. S. 1980, in “Applications of Digital Image Processing to Astronomy”, (ed. D.A. Elliott), p208.
Watanabe, M., Kodaira, K., and Okamura, S. 1982, Astrophys. J. Suppl. 50, 1.
Yamagata, T., Maehara, H., Okamura, S., and Takase, B. 1983, in preparation.
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© 1984 D. Reidei Publishing Company
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Maehara, H., Yamagata, T. (1984). Image Detection System for Schmidt Plates. In: Capaccioli, M. (eds) Astronomy with Schmidt-Type Telescopes. Astrophysics and Space Science Library, vol 110. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6387-0_23
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DOI: https://doi.org/10.1007/978-94-009-6387-0_23
Publisher Name: Springer, Dordrecht
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