TeV Observations of the Variability and Spectrum of Markarian 501

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dc.creatorQuinn, J.
dc.creatorBond, I. H.
dc.creatorBoyle, P. J.
dc.creatorBuckley, J. H.
dc.creatorBradbury, S. M.
dc.creatorBreslin, A. C.
dc.creatorBurdett, A. M.
dc.creatorGordo, J. Bussons
dc.creatorCarter-Lewis, D. A.
dc.creatorCatanese, M.
dc.creatorCawley, M. F.
dc.creatorFegan, D. J.
dc.creatorFinley, J. P.
dc.creatorGaidos, J. A.
dc.creatorHall, A.
dc.creatorHillas, A. M.
dc.creatorKrennrich, F.
dc.creatorLamb, R. C.
dc.creatorLessard, R. W.
dc.creatorMasterson, C.
dc.creatorMcEnery, J. E.
dc.creatorMohanty, G.
dc.creatorMoriarty, P.
dc.creatorRodgers, A. J.
dc.creatorRose, H. J.
dc.creatorSamuelson, F. W.
dc.creatorSembroski, G. H.
dc.creatorSrinivasan, R.
dc.creatorWeeke, T. C.
dc.creatorZweerink, J.
dc.date1997-06-15
dc.date.accessioned2026-07-07T02:23:36Z
dc.date.available2026-07-07T02:23:36Z
dc.descriptionMarkarian 501 is only the second extragalactic source to be detected with high statistical certainty at TeV energies; it is similar in many ways to Markarian 421. The Whipple Observatory gamma-ray telescope has been used to observe the AGN Markarian 501 in 1996 and 1997, the years subsequent to its initial detection. The apparent variability on the one-day time-scale observed in TeV gamma rays in 1995 is confirmed and compared with the variability in Markarian 421. Observations at X-ray and optical wavelengths from 1997 are also presented.
dc.description4 pages, 2 figures, to appear in proceedings of 25th ICRC (Durban)
dc.identifierhttps://arxiv.org/abs/astro-ph/9706142
dc.identifierhttp://arxiv.org/abs/astro-ph/9706142
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11309
dc.subjectAstrophysics
dc.titleTeV Observations of the Variability and Spectrum of Markarian 501
dc.typetext

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