Prospects for detecting and identifying high Galactic latitude EGRET sources at E>50 GeV

Details Prospects for detecting and identifying high Galactic latitude EGRET sources at E>50 GeV Prospects for detecting and identifying high Galactic latitude EGRET sources at E>50 GeV

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aph....11..209b&link_type=abstract

Astroparticle Physics, Volume 11, Issue 1-2, p. 209-212.

Physics

Scientific paper

The majority of EGRET sources remain unidentified with counterparts at any other wavelength. However, a subset of sources at high Galactic latitude are very like to be associated with extragalactic radio sources, and either are blazars or are very similar to them. With the source localization of VERITAS, identification with these radio sources will be much firmer, should they be detected in gamma rays. I will discuss their chances for being detected at E>50 GeV based on the multiwavelength data from representative radio sources which are considered to be good matches to EGRET unidentified objects. I will also discuss implications for the physics and classification of the sources.

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