Multi-wavelength radio monitoring of EGRET sources and candidates

Details Multi-wavelength radio monitoring of EGRET sources and candidates Multi-wavelength radio monitoring of EGRET sources and candidates

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1428e&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1428-1432 (1997).

Computer Science

Radio Sources, Quasars, Active And Peculiar Galaxies And Related Systems, Radio, Microwave

Scientific paper

From several southern hemisphere radio-wavelength monitoring programs, we have compiled multi-wavelength observations of a number of both EGRET-detected sources and sources with similar radio-properties that have not been detected by EGRET. The radio observations were made at 0.8, 2, 5, 8, 90 and 230 GHz, though not all sources were monitored at all wavelengths. The data are compared with EGRET data to the end of Cycle 4 (October 1995) in an effort to confirm previously reported correlations between activity at radio wavelengths and EGRET detections, and to investigate whether the non-EGRET-detected sources were in radio- and gamma-ray-quiet phases during this period.

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