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Pulsar Searches of EGRET Sources

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Type
Preprint
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Submission Date
Identifiers
arXiv ID: astro-ph/0212080
Source
arXiv
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Unknown
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Abstract

The majority of Galactic high-energy gamma-ray sources continue to elude identification. Currently, we have a handful of firm pulsar identifications, one of which is radio quiet, and a few marginal detections, including one millisecond pulsar. Recently, both blind searches of EGRET error boxes and targeted searches of X-ray counterpart candidates have had some success in finding new pulsars. I review these results, and discuss our current program of searching mid-Galactic latitude EGRET error boxes using the Parkes multi-beam system.

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