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Pulsar VLBI Experiment with Kashima(Japan)-Kalyazin(Russia) Baseline

Published online by Cambridge University Press:  12 April 2016

M. Sekido ,
M. Imae ,
Y. Hanado ,
Y. Takahashi ,
Y. Koyama ,
Y.P. Ilyasov ,
A.E. Rodin ,
A.E. Avramenko ,
V.V. Oreshko  and
B.A. Poperechenko
M. Sekido
Affiliation:
Communications Research Laboratory (CRL), Japan.
M. Imae
Affiliation:
Communications Research Laboratory (CRL), Japan.
Y. Hanado
Affiliation:
Communications Research Laboratory (CRL), Japan.
Y. Takahashi
Affiliation:
Communications Research Laboratory (CRL), Japan.
Y. Koyama
Affiliation:
Communications Research Laboratory (CRL), Japan.
Y.P. Ilyasov
Affiliation:
Astro Space Center of P.N.Lebedev Physical Institute, Russia.
A.E. Rodin
Affiliation:
Astro Space Center of P.N.Lebedev Physical Institute, Russia.
A.E. Avramenko
Affiliation:
Astro Space Center of P.N.Lebedev Physical Institute, Russia.
V.V. Oreshko
Affiliation:
Astro Space Center of P.N.Lebedev Physical Institute, Russia.
B.A. Poperechenko
Affiliation:
Special Research Bureau of the Moscow Power Engineering Institute, Russia.

Extract

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Interferometric measurement of a pulsar is one of the most effective techniques to measure accurate source position. Precise measurement of pulsar position will give us the information of proper motion and parallax. Interferometric measurements on pulsars have been carried out, but the number of the pulsars whose position were measured is still smaller than the total number of pulsars. Because newly discovered pulsars are rapidly increasing due to recent intensive systematic surveys. We have started measuring their position by using VLBI between Kashima and Kalyazin. This report shows the results of the first experiment.

Type
Part 2 Precision Measurements
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 117 - 118
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

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