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hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorBRION, E.
dc.contributor.editorF. Combes
dc.contributor.editorD. Barret
dc.contributor.editorT. Contini
dc.contributor.editorF. Meynadier and L. Pagani
dc.date.created2004
dc.date.issued2004
dc.date.conference2004-06-14
dc.description.abstractEnThe CELESTE atmospheric Cherenkov detector ran until June 2004. It has detected several gamma-ray flares of Mrk 421 since 1999. The new data analysis provides better background rejection. We compare our light curves with X-ray data. We significantly improved our understanding of the atmosphere, and of the optical throughput of the detector. This will allow a spectral measurement for Mrk 421 with smaller uncertainties and a more sensitive search for a signal from Mrk 501.
dc.language.isoen
dc.publisherEDP Sciences
dc.source.titleSociété Française d'Astronomie et d'Astrophysique Scientific Highlights 2004
dc.title.enMrk 421 and 501 above 60 GeV: the Influence of CELESTE\'s Energy Scale on the Study of Flares and Spectra
dc.typeChapitre d'ouvrage
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxivastro-ph/0410205
bordeaux.page423
bordeaux.countryFR
bordeaux.title.proceedingSociété Française d'Astronomie et d'Astrophysique Scientific Highlights 2004
bordeaux.conference.cityParis
hal.identifierhal-00012944
hal.version1
hal.conference.end2004-06-18
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00012944v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=Soci%C3%A9t%C3%A9%20Fran%C3%A7aise%20d'Astronomie%20et%20d'Astrophysique%20Scientific%20Highlights%202004&rft.date=2004&rft.spage=423&rft.epage=423&rft.au=BRION,%20E.&rft.genre=unknown


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