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dc.contributor.authorALGABA, Juan-Carlos
dc.contributor.authorLEE, Sang-Sung
dc.contributor.authorKIM, Dae-Won
dc.contributor.authorRANI, Bindu
dc.contributor.authorHODGSON, Jeffrey
dc.contributor.authorKINO, Motoki
dc.contributor.authorTRIPPE, Sascha
dc.contributor.authorPARK, Jong-Ho
dc.contributor.authorZHAO, Guang-Yao
dc.contributor.authorBYUN, Do-Young
dc.contributor.authorGURWELL, Mark
dc.contributor.authorKANG, Sin-Cheol
dc.contributor.authorKIM, Jae-Young
dc.contributor.authorKIM, Jeong-Sook
dc.contributor.authorKIM, Soon-Wook
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorLOTT, Benoit
dc.contributor.authorMIYAZAKI, Atsushi
dc.contributor.authorWAJIMA, Kiyoaki
dc.date.issued2018
dc.description.abstractEnWe present multi-frequency simultaneous VLBI radio observations of the flat spectrum radio quasar 1633+382 (4C 38.41) as part of the interferometric monitoring of γ-ray-bright active galactic nuclei (iMOGABA) program combined with additional observations in the radio, optical, X-rays, and γ-rays carried out during the period 2012 March–2015 August. The monitoring of this source reveals a significant long-lived increase in its activity for approximately two years in the radio bands, which correlates with a similar increase in all other bands from submillimeter to γ-rays. A significant correlation is also found between radio fluxes and simultaneous spectral indices during this period. The study of the discrete correlation function indicates time lags smaller than the uncertainties of ∼40 days among both radio bands and high-energy bands, and a time lag of ∼70 days, with γ-rays leading radio emission. We interpret this as showing that the high-energy and radio fluxes arise from different emitting regions, located at 1 ± 13 and 40 ± 13 pc from the central engine respectively.
dc.language.isoen
dc.subject.engalaxies: jets
dc.subject.engalaxies: individual
dc.subject.engalaxies: active
dc.title.enExploring the Variability of the Flat Spectrum Radio Source 1633+382. I. Phenomenology of the Light Curves
dc.typeArticle de revue
dc.identifier.doi10.3847/1538-4357/aa9e50
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1711.10120
bordeaux.journalAstrophys.J.
bordeaux.page30
bordeaux.volume852
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-01704824
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01704824v1
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