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Pulsar Searches of EGRET Sources

Mallory S. E. Roberts
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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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Mallory S. E. Roberts. 2002-12-03. Pulsar Searches of EGRET Sources. https://arxiv.org/abs/astro-ph/0212080

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