Long term monitoring of bright TeV Blazars with the MAGIC telescope

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dc.creatorGoebel, F.
dc.creatorBackes, M.
dc.creatorBretz, T.
dc.creatorHayashida, M.
dc.creatorHsu, C.
dc.creatorMannheim, K.
dc.creatorMoralejo, A.
dc.creatorRhode, W.
dc.creatorSatalecka, K.
dc.creatorShayduk, M.
dc.creatorTeshima, M.
dc.creatorWagner, R. M.
dc.date2007-09-13
dc.date.accessioned2026-07-07T12:26:50Z
dc.date.available2026-07-07T12:26:50Z
dc.descriptionThe MAGIC telescope has performed long term monitoring observations of the bright TeV Blazars Mrk421, Mrk501 and 1ES1959+650. Up to 40 observations, 30 to 60 minutes each have been performed for each source evenly distributed over the observable period of the year. The sensitivity of MAGIC is sufficient to establish a flux level of 25% of the Crab flux for each measurement. These observations are well suited to trigger multiwavelength ToO observations and the overall collected data allow an unbiased study of the flaring statistics of the observed AGNs.
dc.description4 pages, 4 figures, to appear in the proceedings of the 30th International Cosmic Ray Conference, Merida, July 2007
dc.identifierhttps://arxiv.org/abs/0709.2032
dc.identifierhttp://arxiv.org/abs/0709.2032
dc.identifierProc. 30th Int. Cosm. Ray Conf., R. Caballero et al. (eds.), UNAM, Mexico City, 2008, Vol. 3, pg. 1025-1028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215011
dc.subjectAstrophysics
dc.titleLong term monitoring of bright TeV Blazars with the MAGIC telescope
dc.typetext

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