The Effect of Interstellar and Interplanetary Medium on Precision Pulsar Timing

Details The Effect of Interstellar and Interplanetary Medium on Precision Pulsar Timing The Effect of Interstellar and Interplanetary Medium on Precision Pulsar Timing

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..968..181y&link_type=abstract

ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP Conference Proceedings, Volum

Astronomy and Astrophysics

Astrophysics

2

Pulsars, Interstellar Medium And Nebulae In Milky Way, Solar Wind Plasma, Sources Of Solar Wind, Gravitational Waves: Theory

Scientific paper

The ability to correct dispersion measure (DM) variations due to the interstellar and interplanetary medium is essential for high precision pulsar timing. Here we present an analysis of the variations in DM for 20 millisecond pulsars. We show how they affect pulsar timing residuals and how they can be corrected. We also show that our new model of the solar wind electron density implemented into the TEMPO2 pulsar timing package is more accurate than previous models. This paper summarises the work presented in [1, 2].

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