VHE Gamma Rays from PKS 2155-304

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dc.creatorChadwick, P. M.
dc.creatorLyons, K.
dc.creatorMcComb, T. J. L.
dc.creatorOrford, K. J.
dc.creatorOsborne, J. L.
dc.creatorRayner, S. M.
dc.creatorShaw, S. E.
dc.creatorTurver, K. E.
dc.date1999-06-08
dc.date.accessioned2026-07-07T02:31:54Z
dc.date.available2026-07-07T02:31:54Z
dc.descriptionThe X-ray selected BL Lac PKS 2155-304 has been observed using the University of Durham Mark 6 very high energy gamma ray telescope during 1998. We find no evidence for TeV emission during these recent observations when the X-ray flux was observed to be low. We have reconsidered our measurements made in 1997 November when PKS 2155-304 was in a bright X-ray state and extended X-ray and GeV gamma ray observations were made as part of a multiwavelength campaign. Comparisons are made of the VHE emission during this time with the available data from other wavelengths.
dc.description4 pages, 3 figures, to appear in the Proceedings of 26th International Cosmic Ray Conference (Salt Lake City, 1999)
dc.identifierhttps://arxiv.org/abs/astro-ph/9906132
dc.identifierhttp://arxiv.org/abs/astro-ph/9906132
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14323
dc.subjectAstrophysics
dc.titleVHE Gamma Rays from PKS 2155-304
dc.typetext

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