Tracking dispersion measure variations of timing array pulsars with the GMRT

Research output: Chapter in Book/Report/Conference proceedingConference contribution

  • External authors:
  • Ujjwal Kumar
  • Yashwant Gupta
  • Willem Van Straten
  • Stefan Osłowski
  • Jayanta Roy
  • N. D R Bhat
  • Matthew Bailes

Abstract

We present the results from nearly three years of monitoring of the variations in dispersion measure (DM) along the line-of-sight to 11 millisecond pulsars using the Giant Metrewave Radio Telescope (GMRT). These results demonstrate accuracies of single epoch DM estimates of the order of 5 × 10-4 cm-3 pc. A preliminary comparison with the Parkes Pulsar Timing Array (PPTA) data shows that the measured DM fluctuations are comparable. We show effects of DM variations due to the solar wind and solar corona and compare with the existing models. © 2013 International Astronomical Union.

Bibliographical metadata

Original languageEnglish
Title of host publicationProceedings of the International Astronomical Union|Proc. Int. Astron. Union
Pages432-434
Number of pages2
Volume8
DOIs
Publication statusPublished - Aug 2012

Publication series

NameIAU Symposium