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Correlators for interferometry – Today and Tomorrow

Published online by Cambridge University Press:  12 April 2016

Yoshihiro Chikada*
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano-Ken 384-13, Japan

Abstract

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History of correlators for radio interferrometer is briefly reviewed. Advantages and disadvantages of various methods are discussed and the most appropriate ways are given for various interferrometers. Challenges to the next generation short-wavelength interferrometer are also discussed.

Type
Hardware for Interferometry
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

Chikada, Y. 1981, Nobeyama Radio Observ. Rep., no. 8; also presented at the URSI General Assembly, Washington DC, 1981.Google Scholar
Chikada, Y., Ishiguro, M., Hirabayashi, H., Morimoto, M., Morita, K-I., Kanzawa, T., Iwashita, H., Nakazima, K., Ishikawa, S., Takahashi, T., Handa, K., Kasuga, T., Okumura, S., Miyazawa, T., Nakazuru, T., Miura, K., and Nagasawa, S. 1987, Proc. IEEE, 75, 1203.Google Scholar
Torres, M. 1990, private communication.Google Scholar
Van Vleck, J.H. and Middleton, E. 1966, Proc. IEEE, 54, 2.Google Scholar
Weinreb, S., Barrett, M., Meeks, M.L., and Henry, C. 1963, Nature, 200, 829.CrossRefGoogle Scholar