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

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

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ptti.meet...65h&link_type=abstract

In NASA. Goddard Space Flight Center, The 24th Annual Precise Time and Time Interval (PTTI) Applications and Planning Meeting p

Statistics

Applications

Astrometry, Pulsars, Time Measurement, Very Long Base Interferometry, Correlators, Interferometers

Scientific paper

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.

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