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dc.contributor.authorBRITTO, Richard J.
dc.contributor.authorBUSON, Sara
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorLOTT, Benoît
dc.contributor.authorRAZZAQUE, Soebur
dc.contributor.authorBOTTACINI, Eugenio
dc.date.issued2016
dc.description.abstractEnA prominent outburst of the flat spectrum radio quasar 3C 454.3 was observed in 2014 June with the Fermi Large Area Telescope. This outburst was characterized by a three-stage light-curve pattern—plateau, flare, and post-flare—that occurred from 2014 May to July, in a similar pattern as observed during the exceptional outburst in 2010 November. The highest flux of the outburst reported in this paper occurred during 2014 June 7–29, showing a multiple-peak structure in the light-curves. The average flux in these 22 days was found to be $F[E\gt 100\,\mathrm{MeV}]=(7.2\pm 0.2)\times {10}^{-6}$ ph cm(−)(2) s(−)(1), with a spectral index, for a simple power law, of ${\rm{\Gamma }}=2.04\pm 0.01$. That made this outburst the first γ-ray high state of 3C 454.3 ever to be detected by Fermi with such a hard spectrum over several days. The highest flux was recorded on 2014 June 15, in a 3 hr bin, at MJD 56823.5625, at a level of $F[E\gt 100\,\mathrm{MeV}]=(17.6\pm 1.9)\times {10}^{-6}$ ph cm(−)(2) s(−)(1). The rise time of one of the short subflares was found to be ${T}_{r}=1200\pm 700$ s at MJD = 56827, when the flux increased from 4 to 12 × 10(−)(6) ph cm(−)(2) s(−)(1). Several photons above 20 GeV were collected during this outburst, including one at 45 GeV on MJD 56827, constraining the γ-ray emission region to be located close to the outer boundary of the broad-line region, leading to fast flux variability.
dc.language.isoen
dc.subject.engalaxies: active
dc.subject.engamma rays: galaxies
dc.subject.enquasars: individual
dc.title.enFermi-LAT Observations of the 2014 May–July outburst from 3C 454.3
dc.typeArticle de revue
dc.identifier.doi10.3847/0004-637X/830/2/162
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1511.02280
bordeaux.journalAstrophys.J.
bordeaux.page162
bordeaux.volume830
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-03626539
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03626539v1
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