The CAT Imaging Telescope

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dc.creatorBarrau, A.
dc.creatorBazer-Bachi, R.
dc.creatorCabot, H.
dc.creatorChounet, L. M.
dc.creatorDebiais, G.
dc.creatorDegrange, B.
dc.creatorDezalay, J. P.
dc.creatorDjannati-Atai, A.
dc.creatorDumora, D.
dc.creatorEspigat, P.
dc.creatorFabre, B.
dc.creatorFleury, P.
dc.creatorFontaine, G.
dc.creatorGeorge, R.
dc.creatorGhesquiere, C.
dc.creatorGoret, P.
dc.creatorGouiffes, C.
dc.creatorGrenier, I. A.
dc.creatorIacoucci, L.
dc.creatorBohec, S. Le
dc.creatorMallet, I.
dc.creatorMeynadier, C.
dc.creatorMunz, F.
dc.creatorPalfrey, T. A.
dc.creatorPare, E.
dc.creatorPons, Y.
dc.creatorPunch, M.
dc.creatorQuebert, J.
dc.creatorRagan, K.
dc.creatorRenault, C.
dc.creatorRivoal, M.
dc.creatorRob, L.
dc.creatorSchovanek, P.
dc.creatorSmith, D.
dc.creatorTavernet, J. P.
dc.creatorVrana, J.
dc.date1997-05-30
dc.date.accessioned2026-07-07T02:23:28Z
dc.date.available2026-07-07T02:23:28Z
dc.descriptionThe VHE gamma-ray imaging telescope CAT started taking data in October 1996. Located at the Themis solar site in southern France, it features a 17.7 m^2 Davies-Cotton mirror equipped with 600 PMT camera at the focal plane. The mechanics and optics, the PMTs and the electronics are presented. The performance, based on the first 7 months of operation, is discribed.
dc.description4 pages, 2 figures, Tex, contribution to 25th ICRC Durban
dc.identifierhttps://arxiv.org/abs/astro-ph/9705247
dc.identifierhttp://arxiv.org/abs/astro-ph/9705247
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11258
dc.subjectAstrophysics
dc.titleThe CAT Imaging Telescope
dc.typetext

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