First pulsar VLBI experiment in Japan between Kashima and Usuda

Details First pulsar VLBI experiment in Japan between Kashima and Usuda First pulsar VLBI experiment in Japan between Kashima and Usuda

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasj...46..511h&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 46, no. 5, p. 511-514

Astronomy and Astrophysics

Astronomy

1

Pulsars, Pulse Amplitude, Radiant Flux Density, Radio Astronomy, Very Long Base Interferometry, Computer Programs, Correlators, Gratings, Radio Antennas, Signal To Noise Ratios

Scientific paper

We carried out very long-baseline interferometry (VLBI) experiments on the pulsar PSR 0329+54 in August and November of 1992 by using the Kashima 26 m and the Usuda 64 m antennas. A fringe of a pulsar was detected for the first time in Japan by using newly developed correlation software and the K3 VLBI correlator, which were developed by the Communications Research Laboratory (CRL). To check the gating ability of the correlator, the correlation amplitude was measured for various gating times, from which we derived the gating time that produces the highest signal-to-noise ratio.

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