Timing Observation of the Millisecond Pulsar PSR i 1937 + 21 Using the Kashima 34 m-Antenna

Details Timing Observation of the Millisecond Pulsar PSR i 1937 + 21 Using the Kashima 34 m-Antenna Timing Observation of the Millisecond Pulsar PSR i 1937 + 21 Using the Kashima 34 m-Antenna

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pasj...54..305h&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.54, No.2, pp.305-313

Astronomy and Astrophysics

Astronomy

4

Radio Continuum: Stars, Stars: Pulsars: Individual (Psr 1937 + 21), Telescopes, Time

Scientific paper

Communications Research Laboratory (CRL) has developed a precise measurement system for millisecond pulsar timing using the 34-m antenna at Kashima Space Research Center, one of the smallest antennas for millisecond pulsar observations. Timing observations of the millisecond pulsar PSR1937 + 21 have been ongoing since 1997 November at Kashima. From observational data of almost three years, we obtained a timing accuracy of 2.65 μs from daily-averaged residuals, and found the frequency stability to be about 1 × 10-13 over a period of one year. This result confirms the observational sensitivity of our system, and shows the possibility of constructing a pulsar time scale by using a system with a small antenna.

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