A Time Differencing Method for Finding Pulsars in Gamma-Ray Data

Details A Time Differencing Method for Finding Pulsars in Gamma-Ray Data A Time Differencing Method for Finding Pulsars in Gamma-Ray Data

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0124z&link_type=abstract

American Astronomical Society, HEAD meeting #9, #1.24; Bulletin of the American Astronomical Society, Vol. 38, p.333

Astronomy and Astrophysics

Astronomy

Scientific paper

Several theoretical models for the Gamma-Ray pulsar population predict a large fraction of radio quiet Gamma-Ray pulsars. The upcoming GLAST mission will detect several hundred radio quiet Gamma-Ray pulsars. We present a fast method for finding the spin parameters of Gamma-Ray pulsars in a blind search. The sensitivity of our new method was determined with a simple pulsar simulation and simulated GLAST data. We also demonstrate the benefits of the new method on EGRET data.

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