Statistics – Applications
Scientific paper
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.
Fujisawa Katsuki
Hama Shin'ichi
Hanado Yuko
Hirabayashi Hisahi
Imae Masato
No associations
LandOfFree
Pulsar astrometry by using VLBI (PSR0329 between Kashima 26mPhi and Usuda 64mPhi) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Pulsar astrometry by using VLBI (PSR0329 between Kashima 26mPhi and Usuda 64mPhi), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsar astrometry by using VLBI (PSR0329 between Kashima 26mPhi and Usuda 64mPhi) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1336368