Very high energy gamma rays from PKS 2155-304

Citation
Pm. Chadwick et al., Very high energy gamma rays from PKS 2155-304, ASTROPHYS J, 513(1), 1999, pp. 161-167
Citations number
44
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
513
Issue
1
Year of publication
1999
Part
1
Pages
161 - 167
Database
ISI
SICI code
0004-637X(19990301)513:1<161:VHEGRF>2.0.ZU;2-C
Abstract
The close X-ray-selected BL Lac PKS 2155-304 has been observed using the Un iversity of Durham Mark 6 very high energy (VHE) gamma-ray telescope during 1996 September/October/November and 1997 October/November, VHE gamma rays with energy more than 300 GeV were detected from this object with a time-av eraged integral flux of (4.2 +/- 0.7(stat) +/- 2.0(sys)) x 10(-11) cm(-2) s (-1). There is evidence for VHE gamma-ray emission during our observations in 1996 September and 1997 October/November, with the strongest emission be ing detected in 1997 November, when the object was producing the largest fl ux ever recorded in high-energy X-rays and it was detected as a source of g amma rays of energy greater than 100 MeV. The VHE and X-ray fluxes show evi dence of a correlation.