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http://hdl.handle.net/20.500.12386/28803
Titolo: | AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C +71.07 in outburst | Autori: | VERCELLONE, STEFANO ROMANO, Patrizia PIANO, Giovanni VITTORINI, VALERIO Donnarumma, I. Munar-Adrover, P. RAITERI, Claudia Maria VILLATA, Massimo VERRECCHIA, Francesco LUCARELLI, Fabrizio PITTORI, Carlotta BULGARELLI, ANDREA FIORETTI, VALENTINA TAVANI, MARCO Acosta-Pulido, J. A. Agudo, I. Arkharov, A. A. Bach, U. Bachev, R. Borman, G. A. Butuzova, M. S. CARNERERO MARTIN, Maria Isabel Casadio, C. Damljanovic, G. D'AMMANDO, FILIPPO DI PAOLA, Andrea Doroshenko, V. T. Efimova, N. V. Ehgamberdiev, Sh. A. GIROLETTI, MARCELLO Gómez, J. L. Grishina, T. S. Järvelä, E. Klimanov, S. A. Kopatskaya, E. N. Kurtanidze, O. M. Lähteenmäki, A. Larionov, V. M. Larionova, L. V. Mihov, B. Mirzaqulov, D. O. Molina, S. N. Morozova, D. A. Nazarov, S. V. ORIENTI, Monica RIGHINI, SIMONA Savchenko, S. S. Semkov, E. Slavcheva-Mihova, L. Strigachev, A. Tornikoski, M. Troitskaya, Yu. V. Vince, O. Cattaneo, P. W. Colafrancesco, S. Longo, F. Morselli, A. Paoletti, F. PARMIGGIANI, NICOLO |
Data pubblicazione: | 2019 | Rivista: | ASTRONOMY & ASTROPHYSICS | Numero: | 621 | Da pagina:: | A82 | Abstract: | Context. The flat-spectrum radio quasar 4C +71.07 is a high-redshift (z = 2.172), γ-loud blazar whose optical emission is dominated by thermal radiation from the accretion disc. <BR /> Aims: 4C +71.07 has been detected in outburst twice by the AGILE γ-ray satellite during the period from the end of October to mid-November 2015, when it reached a γ-ray flux of the order of F(E > 100 MeV)=(1.2 ± 0.3)×10<SUP>-6</SUP> photons cm<SUP>-2</SUP> s<SUP>-1</SUP> and F(E > 100 MeV)=(3.1 ± 0.6)×10<SUP>-6</SUP> photons cm<SUP>-2</SUP> s<SUP>-1</SUP>, respectively, allowing us to investigate the properties of the jet and the emission region. <BR /> Methods: We investigated its spectral energy distribution by means of almost-simultaneous observations covering the cm, mm, near-infrared, optical, ultraviolet, X-ray, and γ-ray energy bands obtained by the GASP-WEBT Consortium and the Swift, AGILE, and Fermi satellites. <BR /> Results: The spectral energy distribution of the second γ-ray flare (whose energy coverage is more dense) can be modelled by means of a one-zone leptonic model, yielding a total jet power of about 4 × 10<SUP>47</SUP> erg s<SUP>-1</SUP>. <BR /> Conclusions: During the most prominent γ-ray flaring period our model is consistent with a dissipation region within the broad-line region. Moreover, this class of high-redshift, flat-spectrum radio quasars with high-mass black holes might be good targets for future γ-ray satellites such as e-ASTROGAM. <P />Partly based on data taken and assembled by the WEBT collaboration and stored in the WEBT archive at the Osservatorio Astrofisico di Torino - INAF (<A href="http://www.oato.inaf.it/blazars/webt">http://www.oato.inaf.it/blazars/webt</A>). | URI: | http://hdl.handle.net/20.500.12386/28803 | URL: | https://www.aanda.org/articles/aa/abs/2019/01/aa32532-17/aa32532-17.html | ISSN: | 0004-6361 | DOI: | 10.1051/0004-6361/201732532 | Bibcode ADS: | 2019A&A...621A..82V | Fulltext: | open |
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