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Timing Observations of PSR B1937+21 at CRL

Published online by Cambridge University Press:  19 July 2016

Y. Hanado ,
Y. Shibuya ,
F. Nakagawa ,
M. Sekido ,
M. Hosokawa  and
M. Imae
Y. Hanado
Affiliation:
Communications Research Laboratory (CRL), 4-2-1, Nukui-Kita, Koganei, Tokyo 184-8795, Japan
Y. Shibuya
Affiliation:
Communications Research Laboratory (CRL), 4-2-1, Nukui-Kita, Koganei, Tokyo 184-8795, Japan
F. Nakagawa
Affiliation:
Communications Research Laboratory (CRL), 4-2-1, Nukui-Kita, Koganei, Tokyo 184-8795, Japan
M. Sekido
Affiliation:
Communications Research Laboratory (CRL), 4-2-1, Nukui-Kita, Koganei, Tokyo 184-8795, Japan
M. Hosokawa
Affiliation:
Communications Research Laboratory (CRL), 4-2-1, Nukui-Kita, Koganei, Tokyo 184-8795, Japan
M. Imae
Affiliation:
Communications Research Laboratory (CRL), 4-2-1, Nukui-Kita, Koganei, Tokyo 184-8795, Japan

Abstract

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Pulsar parameters of PSR B1937+21 acquired from observations at the Kashima 34-m antenna over five years are consistent with published reports. The frequency stability is 2 × 10−14 over the data span of 6.5 years using Kashima data combined with Parkes data.

Type
Part 10: Radio Pulsar Timing
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 437 - 438
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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