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The Conversion from the B1950 FK4-Based Position to the J2000 Position of Celestial Objects

Published online by Cambridge University Press:  04 August 2017

S. Aoki ,
M. Sôma ,
K. Nakajima ,
Y. Niimi ,
M. Fujishita  and
Y. Takahashi
S. Aoki
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
M. Sôma
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
K. Nakajima
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
Y. Niimi
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
M. Fujishita
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
Y. Takahashi
Affiliation:
1Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan

Extract

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We present here the fundamental idea of the conversion method between old and new reference frameworks. Some practical applications are made for the optical observations for Tokyo PZT. The method can be also applied to the conversion of radio sources where we have met a great difficulty in performing the conversion because of no citation of observation epochs in general. We discuss their necessity in order to establish a concrete compilation of the position of the radio sources.

Type
I. Reduction Technique
Information
Symposium - International Astronomical Union , Volume 109: Astrometric Techniques , 1986 , pp. 123 - 131
Copyright
Copyright © Reidel 1986 

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