A mathematical method for the de-dispersion of the pulsar profile

Details A mathematical method for the de-dispersion of the pulsar profile A mathematical method for the de-dispersion of the pulsar profile

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010scchg..53s.228y&link_type=abstract

Science China Physics, Mechanics and Astronomy, Volume 53, Issue 1, pp.228-230

Astronomy and Astrophysics

Astronomy

Pulsar, Dispersion Measure, Interstellar Medium

Scientific paper

This paper presents a mathematical method for de-dispersion of average
pulsar profiles. We applied this method to four dispersed pulsar
profiles. The results revealed that this method significantly removed
the dispersion broadening and the pulse widths were reduced by about 7%
to 27%, depending on the magnitude of the pulsar dispersion measure.

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