Pulsar Astrometry by Using VLBl (PSR0329 between Kashima 26mo & Usuda 64mo)

S. Hama, H. Kiuchi, Y. Hanado, Y. Takahashi, M. Imae, K. Fujisawa. H . Hirabayashi, H. Kobayashi

Abstract:	Communications Research Laboratory (CRL). carried out a VLBl (Very Long Baseline Interferometer) experiment, of the pulsar 0329+54 on November in 1992 between Kashima 26mo and Usuda 64mo. We got a correlation for it by using K-3 VLBl correlator. which was developed by CRL. Though we observed a slow pulsar this time, we are going to make millisecond pulsar experiments by making good use of this result and by using K-4 correlator which is under developing in CRL. Its result will give us precise positions and proper motions of pulsars which are useful for obtaining precise pulsar timing.
Published in:	Proceedings of the 24th Annual Precise Time and Time Interval Systems and Applications Meeting December 1 - 3, 1992 Ritz-Carlton Hotel McLean, Virginia
Pages:	65 - 72
Cite this article:	Hama, S., Kiuchi, H., Hanado, Y., Takahashi, Y., Imae, M., Hirabayashi, K. Fujisawa. H ., Kobayashi, H., "Pulsar Astrometry by Using VLBl (PSR0329 between Kashima 26mo & Usuda 64mo)," Proceedings of the 24th Annual Precise Time and Time Interval Systems and Applications Meeting, McLean, Virginia, December 1992, pp. 65-72.
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