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dc.contributor.authorDERMER, C.D.
dc.contributor.authorCAVADINI, M.
dc.contributor.authorRAZZAQUE, S.
dc.contributor.authorFINKE, J.D.
dc.contributor.authorCHIANG, J.
hal.structure.identifierGLAST
dc.contributor.authorLOTT, B.
dc.date.issued2011-06-01
dc.identifier.issn2041-8205
dc.description.abstractEnRecent claims that the strength BIGMF of the intergalactic magnetic field (IGMF) is 10−15 G are based on upper limits to the expected cascade flux in the GeV band produced by blazar TeV photons absorbed by the extragalactic background light. This limit depends on an assumption that themean blazar TeV flux remains constant on timescales 2(BIGMF/10−18G)2/(E/10 GeV)2 yr for an IGMF coherence length ≈1 Mpc, where E is the measured photon energy. Restricting TeV activity of 1ES 0229+200 to ≈3-4 years during which the source has been observed leads to a more robust lower limit of BIGMF 10−18 G, which can be larger by an order of magnitude if the intrinsic source flux above ≈5-10 TeV from 1ES 0229+200 is strong.
dc.language.isoen
dc.publisherBristol : IOP Publishing
dc.subject.engalaxies: jets
dc.subject.engamma rays: galaxies
dc.subject.enradiation mechanisms: non-thermal
dc.title.enTime delay of cascade radiation for TeV blazars and the measurement of the intergalactic magnetic field
dc.typeArticle de revue
dc.identifier.doi10.1088/2041-8205/733/2/L21
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.identifier.arxiv1011.6660
bordeaux.journalThe Astrophysical journal letters
bordeaux.pageL21
bordeaux.volume733
bordeaux.peerReviewedoui
hal.identifierin2p3-00654631
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00654631v1
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