Study of Mrk 501 above 60 GeV with CELESTE

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dc.creatorBrion, E.
dc.creatorcollaboration, the CELESTE
dc.date2005-09-16
dc.date.accessioned2026-07-07T02:18:41Z
dc.date.available2026-07-07T02:18:41Z
dc.descriptionThe CELESTE atmospheric Cherenkov detector, running until June 2004 at the Themis solar facility, has taken data on compact sources such as pulsars and blazars. We will take stock of the experiment, in particular regarding the latest improvements of the detector simulation and data analysis. These changes provide us with a new analysis of old data with smaller uncertainties. We present here the evidence for a weak signal from Mrk 501 in 2000-2001.
dc.description4 pages, 8 figures, proc. of the 22nd Texas Symposium on Relativistic Astrophysics at Stanford University, US, December 13-17, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0509498
dc.identifierhttp://arxiv.org/abs/astro-ph/0509498
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9583
dc.subjectAstrophysics
dc.titleStudy of Mrk 501 above 60 GeV with CELESTE
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