Pulsar Time Scale: Gravitational Time Delay in Pulsar Timing

Details Pulsar Time Scale: Gravitational Time Delay in Pulsar Timing Pulsar Time Scale: Gravitational Time Delay in Pulsar Timing

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999crlrv..45..151h&link_type=abstract

Review of the Communications Research Laboratory, vol. 45, p. 151

Mathematics

Probability

Pulsars, Time Lag, Gravitational Effects, Time Measurement, Stellar Mass, Astrometry, Relativity, Celestial Reference Systems

Scientific paper

We propose the inclusion of a new correction term, the gravitational time delay effect caused by an intervening star, in the analysis of pulsar timing observation. The analysis of this effect will not only help to stabilize the pulsar time but also provide a new way to determine the mass of the intervening star directly. In 10 years observation with the TOA accuracy of 200 ns, the probability would be more than 1% for a pulsar of a few kpc distance.

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