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dc.contributor.authorMaraschi, L.
dc.contributor.authorFossati, G.
dc.contributor.authorTavecchio, F.
dc.contributor.authorChiappetti, L.
dc.contributor.authorCelotti, A.
dc.contributor.authorGhisellini, G.
dc.contributor.authorGrandi, P.
dc.contributor.authorPian, E.
dc.contributor.authorTagliaferri, G.
dc.contributor.authorTreves, A.
dc.contributor.authorBreslin, A. C.
dc.contributor.authorBuckley, J. H.
dc.contributor.authorCarter-Lewis, D. A.
dc.contributor.authorCatanese, M.
dc.contributor.authorCawley, M. F.
dc.contributor.authorFegan, D. J.
dc.contributor.authorFegan, S.
dc.contributor.authorFinley, J.
dc.contributor.authorGaidos, J.
dc.contributor.authorHall, T.
dc.contributor.authorHillas, A. M.
dc.contributor.authorKrennrich, F.
dc.contributor.authorLessard, R. W.
dc.contributor.authorMasterson, C.
dc.contributor.authorMoriarty, P.
dc.contributor.authorQuinn, J.
dc.contributor.authorRose, J.
dc.contributor.authorSamuelson, F.
dc.contributor.authorWeekes, T. C.
dc.contributor.authorUrry, C. M.
dc.contributor.authorTakahashi, T.
dc.date.accessioned2018-08-24T08:25:33Z
dc.date.available2018-08-24T08:25:33Z
dc.date.issued1999-12-01
dc.identifier.citationMaraschi, L. Fossati, G.; Tavecchio, F.; Chiappetti, L.; Celotti, A.; Ghisellini, G.; Grandi, P.; Pian, E.; Tagliaferri, G.; Treves, A.; Breslin, A. C.; Buckley, J. H.; Carter-Lewis, D. A.; Catanese, M.; Cawley, M. F.; Fegan, D. J.; Fegan, S.; Finley, J.; Gaidos, J.; Hall, T.; Hillas, A. M.; Krennrich, F.; Lessard, R. W.; Masterson, C.; Moriarty, P.; Quinn, J.; Rose, J.; Samuelson, F.; Weekes, T. C.; Urry, C. M.; Takahashi, T. (1999). Simultaneous x-ray and t[clc]e[/clc]v observations of a rapid flare from markarian 421. The Astrophysical Journal 526 (2), L81-L84
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/10379/9486
dc.description.abstractMrk 421 was observed for about 2 days with BeppoSAX in 1998 April as part of a worldwide multiwavelength campaign. A large, well-defined flare was observed in X-rays. The same flare was observed simultaneously at TeV energies by the Whipple Observatory gamma-ray telescope. These data provide (1) the first evidence that the X-ray and TeV intensities are well correlated on timescales of hours and (2) the first exactly simultaneous X-ray and TeV spectra. The results imply that the X-ray and TeV photons derive from the same region and from the same population of relativistic electrons. 'The physical parameters deduced from a homogeneous synchrotron self-Compton model for the spectral energy distribution yield electron cooling times close to the observed variability timescales.
dc.publisherIOP Publishing
dc.relation.ispartofThe Astrophysical Journal
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Ireland
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/3.0/ie/
dc.subjectbl lacertae objects : individual (markarian 421)
dc.subjectgalaxies : active
dc.subjectgalaxies : jets
dc.subjectgamma rays : observations
dc.subjectx-rays : galaxies
dc.subjectlacertae object markarian-421
dc.subjectspectral energy-distributions
dc.subjectactive galaxy markarian-421
dc.subjectmultiwavelength observations
dc.subjectblazars
dc.subjectvariability
dc.subjectemission
dc.subjectphotons
dc.subjectbursts
dc.subjectjets
dc.titleSimultaneous x-ray and t[clc]e[/clc]v observations of a rapid flare from markarian 421
dc.typeArticle
dc.identifier.doi10.1086/312370
dc.local.publishedsourcehttp://iopscience.iop.org/article/10.1086/312370/pdf
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