Timing of New Pulsars from Re-Analysis of the Parkes Multibeam Pulsar Survey

Details Timing of New Pulsars from Re-Analysis of the Parkes Multibeam Pulsar Survey Timing of New Pulsars from Re-Analysis of the Parkes Multibeam Pulsar Survey

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..563k&link_type=abstract

ATNF proposal P559, Semester: October, 2006

Physics

Galactic, Parkes

Scientific paper

Re-analysis of the Parkes Multibeam Pulsar Survey has lead to the discovery of 22 new pulsar candidates. Timing observations are an essential to fully exploit the scientific benefits of these discoveries. It is imperative that the observations be spaced approximately once per month apart, as described in the science case. The sources will be visible during the 12:00-20:00 LST range and the project should be scheduled within this interval.

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