Optical studies of potential counterparts for unidentified EGRET sources

Details Optical studies of potential counterparts for unidentified EGRET sources Optical studies of potential counterparts for unidentified EGRET sources

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..494c&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 494-498 (2000).

Computer Science

4

Gamma-Ray Sources, Gamma-Ray Bursts, Visible

Scientific paper

We present optical observations of candidate X-ray counterparts for the EGRET sources 3EG J2020+4017, 3EG J0010+7309 and 3EG J1835+5918. Preliminary spectroscopic observations of the late-type star coincident with the X-ray counterpart of 3EG J2020+4017, the γ-Cygni source, show no evidence of binariety. In the case of 3EG J0010+7309, the CTA-1 source, we performed deep optical imaging, finding a red V~22 magnitude object inside the ROSAT contour. Finally, a detailed analysis of optical observations of several X-ray sources within the EGRET error box of 3EG J1835+5918 is presented. .

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