Gamma ray pulsar analysis from photon pobability maps

Details Gamma ray pulsar analysis from photon pobability maps Gamma ray pulsar analysis from photon pobability maps

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sdgg.nasa.....b&link_type=abstract

In its Gamma-Ray Spectroscopy: The Diffuse Galactic Glow 6 p (SEE N92-16968 07-93)

Mathematics

Probability

Astronomical Maps, Detection, Galactic Radiation, Gamma Rays, Photons, Probability Distribution Functions, Pulsars, Cos-B Satellite, Data Processing, Probability Theory

Scientific paper

We present a new method of analyzing skymap-type gamma ray data. Each photon event is replaced by a probability distribution on the sky corresponding to the observing instrument's point spread function. The skymap produced by this process may be used for source detection or identification. Most important, the use of these photon weights for pulsar analysis promises significant improvement over traditional techniques.

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