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Review of the solar array telescopes

hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorSMITH, D.A.
dc.contributor.editorB. Degrange, G. Fontaine
dc.date.created2005
dc.date.issued2005
dc.date.conference2005-04-27
dc.description.abstractEnFor several years the only experiments sensitive to astrophysical gamma rays with energies beyond the reach of EGRET but below that the Cherenkov imaging telescopes have been the "solar towar" detectors. They use > 2000 m$^{2}$ mirror areas to sample the Cherenkov wavefront generated by <100 GeV gamma rays, obtained Crab sensitivities of more than 6 $\sigma$ in one ON-source hour. I will review the history of the solar tower Cherenkov experiments from 1992 to the present and their key design features. I will describe some successful analysis strategies, then summarize the principal results obtained.
dc.language.isoen
dc.publisherEcole Polytechnique Palaiseau
dc.source.titleTowards a Network of Atmospheric Cherenkov Detectors VII
dc.title.enReview of the solar array telescopes
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
bordeaux.page67-79
bordeaux.countryFR
bordeaux.title.proceedingTowards a Network of Atmospheric Cherenkov Detectors VII
bordeaux.conference.cityPalaiseau
bordeaux.peerReviewedoui
hal.identifierin2p3-00025735
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2005-04-29
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00025735v1
bordeaux.COinSctx_ver=Z39.88-2004&amp;rft_val_fmt=info:ofi/fmt:kev:mtx:journal&amp;rft.btitle=Towards%20a%20Network%20of%20Atmospheric%20Cherenkov%20Detectors%20VII&amp;rft.date=2005&amp;rft.spage=67-79&amp;rft.epage=67-79&amp;rft.au=SMITH,%20D.A.&amp;rft.genre=unknown


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