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dc.contributor.authorAhnen, M.-
dc.contributor.authorAnsoldi, S.-
dc.contributor.authorAntonelli, L.-
dc.contributor.authorAntoranz, P.-
dc.contributor.authorArcaro, C.-
dc.contributor.authorBabic, A.-
dc.contributor.authorBanerjee, B.-
dc.contributor.authorBangale, P.-
dc.contributor.authorBarres De Almeida, U.-
dc.contributor.authorBarrio, J.-
dc.contributor.authorBecerra González, J.-
dc.contributor.authorBednarek, W.-
dc.contributor.authorBernardini, E.-
dc.contributor.authorBerti, A.-
dc.contributor.authorBiasuzzi, B.-
dc.contributor.authorBiland, A.-
dc.contributor.authorBlanch, O.-
dc.contributor.authorBonnefoy, S.-
dc.contributor.authorBonnoli, G.-
dc.contributor.authorBorracci, F.-
dc.contributor.authoret al.-
dc.identifier.citationAstronomy and Astrophysics: a European journal, 2016; 595:A98-1-A98-11-
dc.description.abstractContext. QSO B0218+357 is a gravitationally lensed blazar located at a redshift of 0.944. The gravitational lensing splits the emitted radiation into two components that are spatially indistinguishable by gamma-ray instruments, but separated by a 10–12 day delay. In July 2014, QSO B0218+357 experienced a violent flare observed by the Fermi-LAT and followed by the MAGIC telescopes.Aims. The spectral energy distribution of QSO B0218+357 can give information on the energetics of z ~ 1 very high energy gamma-ray sources. Moreover the gamma-ray emission can also be used as a probe of the extragalactic background light at z ~ 1. Methods. MAGIC performed observations of QSO B0218+357 during the expected arrival time of the delayed component of the emission. The MAGIC and Fermi-LAT observations were accompanied by quasi-simultaneous optical data from the KVA telescope and X-ray observations by Swift-XRT. We construct a multiwavelength spectral energy distribution of QSO B0218+357 and use it to model the source. The GeV and sub-TeV data obtained by Fermi-LAT and MAGIC are used to set constraints on the extragalactic background light. Results. Very high energy gamma-ray emission was detected from the direction of QSO B0218+357 by the MAGIC telescopes during the expected time of arrival of the trailing component of the flare, making it the farthest very high energy gamma-ray source detected to date. The observed emission spans the energy range from 65 to 175 GeV. The combined MAGIC and Fermi-LAT spectral energy distribution of QSO B0218+357 is consistent with current extragalactic background light models. The broadband emission can be modeled in the framework of a two-zone external Compton scenario, where the GeV emission comes from an emission region in the jet, located outside the broad line region.-
dc.description.statementofresponsibilityM. L. Ahnen, S. Ansoldi, L. A. Antonelli, P. Antoranz, C. Arcaro ... Sabrina Einecke ... et al.-
dc.publisherEDP Sciences-
dc.rights© ESO 2016-
dc.subjectgamma rays: galaxies – gravitational lensing: strong – galaxies: jets – radiation mechanisms: non-thermal – quasars: individual: QSO B0218+357-
dc.titleDetection of very high energy gamma-ray emission from the gravitationally lensed blazar QSO B0218+357 with the MAGIC telescopes-
dc.typeJournal article-
dc.identifier.orcidEinecke, S. [0000-0001-9687-8237]-
Appears in Collections:Aurora harvest 8
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