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Pulsar astrometry by using VLBI (PSR0329 between Kashima 26mPhi and Usuda 64mPhi) (1993)

Hirabayashi, H. ; Kiuchi, H. ; Takahashi, Y. ; [et al.]

In: CASI

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Publication Date: 2004-12-03

Description: Communications Research Laboratory (CRL) carried out a VLBI (Very Long Baseline Interferometer) experiment of the Pulsar 0329 plus 54 on November in 1992 between Kashima 26mPhi and Usuda 64mPhi. We got a correlation for it by using K-3 VLBI 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.

Keywords: ASTRONOMY

Type: NASA. Goddard Space Flight Center, The 24th Annual Precise Time and Time Interval (PTTI) Applications and Planning Meeting; p 65-72

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