Arrival-time analysis for a millisecond pulsar

Details Arrival-time analysis for a millisecond pulsar Arrival-time analysis for a millisecond pulsar

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984japa....5..369b&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0260-6335), vol. 5, Dec. 1984, p. 369-388. Research supported by the Alfred P. Sloan

Statistics

Computation

67

Gravitational Waves, Noise Spectra, Pulsars, Stellar Spectra, Background Radiation, Computational Astrophysics, Power Spectra, Time Measurement, White Noise

Scientific paper

An attempt is made to develop the analysis of pulsar arrival times, in order to estimate the sensitivity of fast pulsars as detectors of gravitational radiation and dispersion-measure fluctuations, under the assumption that they remain as good in their clocking functions as is indicated by present observations. Also explored are the limits of the use of such accurate arrival times to measure pulsar spin-down, position, proper motion, and parallax distance, in the presence of a given noise spectrum. The results obtained are applied to PSR 1937 + 214, yielding quantitative estimates of its sensitivity to gravitational wave, interstellar electron density fluctuation, and intrinsic pulsar noise sources.

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