Pulsar Searches of EGRET Sources

dc.creatorRoberts, Mallory S. E.
dc.date2002-12-03
dc.date.accessioned2026-07-25T18:51:53Z
dc.descriptionThe 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.
dc.description4 pages, to appear in the proceedings of the conference "Radio Pulsars" held in Chania, Crete, Sept. 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0212080
dc.identifierhttp://arxiv.org/abs/astro-ph/0212080
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/59172
dc.subjectAstrophysics
dc.titlePulsar Searches of EGRET Sources
dc.typetext

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