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FältnamnIndikatorerMetadata
00009158naa a2201357 4500
001oai:DiVA.org:lnu-42774
003SwePub
008150423s2015 | |||||||||||000 ||eng|
009oai:DiVA.org:kth-163484
024a https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-427742 URI
024a https://doi.org/10.1093/mnras/stu22512 DOI
024a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1634842 URI
040 a (SwePub)lnud (SwePub)kth
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a D’Ammando, F.u Universitá degli Studi di Bologna, Italy ; INAF – Istituto di Radioastronomia, Italy,Pennsylvania State University, USA,University of California, USA4 aut
2451 0a The most powerful flaring activity from the NLSy1 PMN J0948+0022
264 c 2014-11-27
264 1b Oxford University Press,c 2015
338 a print2 rdacarrier
500 a QC 20150407
520 a We report on multifrequency observations performed during 2012 December–2013 August of the first narrow-line Seyfert 1 galaxy detected in γ-rays, PMN J0948+0022 (z = 0.5846). A γ-ray flare was observed by the Large Area Telescope on board Fermi during 2012 December–2013 January, reaching a daily peak flux in the 0.1–100 GeV energy range of (155 ± 31) × 10−8 ph cm−2 s−1 on 2013 January 1, corresponding to an apparent isotropic luminosity of ∼1.5 × 1048 erg s−1. The γ-ray flaring period triggered Swift and Very Energetic Radiation Imaging Telescope Array System (VERITAS) observations in addition to radio and optical monitoring by Owens Valley Radio Observatory, Monitoring Of Jets in Active galactic nuclei with VLBA Experiments, and Catalina Real-time Transient Survey. A strong flare was observed in optical, UV, and X-rays on 2012 December 30, quasi-simultaneously to the γ-ray flare, reaching a record flux for this source from optical to γ-rays. VERITAS observations at very high energy (E > 100 GeV) during 2013 January 6–17 resulted in an upper limit of F>0.2 TeV < 4.0 × 10−12 ph cm−2 s−1. We compared the spectral energy distribution (SED) of the flaring state in 2013 January with that of an intermediate state observed in 2011. The two SEDs, modelled as synchrotron emission and an external Compton scattering of seed photons from a dust torus, can be modelled by changing both the electron distribution parameters and the magnetic field.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a galaxies: active
653 a galaxies: individual: PMN J0948+0022
653 a galaxies: nuclei
653 a galaxies: Seyfert
653 a gamma-rays: general
653 a Astropartikelfysik
653 a Astroparticle Physics
700a Orienti, M.u INAF – Istituto di Radioastronomia, Italy4 aut
700a Finke, J.u U.S. Naval Research Laboratory, USA,Purdue University, USA4 aut
700a Raiteri, C. M.u INAF – Osservatorio Astrofisico di Torino, Italy,Harvard-Smithsonian Center for Astrophysics, USA,Columbia University, USA4 aut
700a Hovatta, T.u California Institute of Technology, USA4 aut
700a Larsson, Josefinu KTH,Partikel- och astropartikelfysik,Royal Institute of Technology, Sweden,Purdue University, USA4 aut0 (Swepub:kth)u12o773l
700a Max-Moerbeck, W.u National Radio Astronomy Observatory (NRAO), USA4 aut
700a Perkins, J.u NASA Goddard Space Flight Center, USA4 aut
700a Readhead, A. C. S.u California Institute of Technology, USA4 aut
700a Richards, J. L.u Purdue University, USA4 aut
700a Beilicke, M.u Washington University, USA4 aut
700a Benbow, W.u Harvard-Smithsonian Center for Astrophysics, USA4 aut
700a Berger, K.u University of Delaware, USA4 aut
700a Bird, R.u University College Dublin, Ireland4 aut
700a Bugaev, V.u Washington University, USA4 aut
700a Cardenzana, J. V.u Iowa State University, USA4 aut
700a Cerruti, M.u Harvard-Smithsonian Center for Astrophysics, USA4 aut
700a Chen, X.u University of Potsdam, Germany ; DESY, Germany4 aut
700a Ciupik, L.u Adler Planetarium and Astronomy Museum, USA4 aut
700a Dickinson, H. J.u Iowa State University, USA,University of Delaware, USA4 aut
700a Eisch, J. D.u Iowa State University, USA4 aut
700a Errando, M.u Columbia University, USA4 aut
700a Falcone, A.u Pennsylvania State University, USA4 aut
700a Finley, J. P.u Purdue University, USA4 aut
700a Fleischhack, H.u DESY, Germany4 aut
700a Fortin, P.u Harvard-Smithsonian Center for Astrophysics, USA4 aut
700a Fortson, L.u University of Minnesota, USA4 aut
700a Furniss, A.u University of California, USA4 aut
700a Gerard, L.u DESY, Germany4 aut
700a Gillanders, G. H.u National University of Ireland Galway, Ireland,Adler Planetarium and Astronomy Museum, USA,Purdue University, USA4 aut
700a Griffiths, S. T.u University of Iowa, USA4 aut
700a Grube, J.u Adler Planetarium and Astronomy Museum, USA4 aut
700a Gyuk, G.u Adler Planetarium and Astronomy Museum, USA,DESY, Germany,Georgia Institute of Technology, USA4 aut
700a Håkansson, N.u University of Potsdam, Germany4 aut
700a Holder, J.u University of Delaware, USA4 aut
700a Humensky, T. B.u Columbia University, USA4 aut
700a Kar, P.u University of Utah, USA4 aut
700a Kertzman, M.u DePauw University, USA,Georgia Institute of Technology, USA4 aut
700a Khassen, Y.u University College Dublin, Ireland4 aut
700a Kieda, D.u University of Utah, USA4 aut
700a Krennrich, F.u Iowa State University, USA4 aut
700a Kumar, S.u University of Delaware, USA4 aut
700a Lang, M. J.u National University of Ireland Galway, Ireland4 aut
700a Maier, G.u DESY, Germany4 aut
700a McCann, A.u University of Chicago, USA4 aut
700a Meagher, K.u Georgia Institute of Technology, USA4 aut
700a Moriarty, P.u National University of Ireland Galway, Ireland,University of Potsdam, Germany ; DESY, Germany4 aut
700a Mukherjee, R.u Columbia University, USA4 aut
700a Nieto, D.u Columbia University, USA4 aut
700a de Bhróithe, A. O.u DESY, Germany4 aut
700a Ong, R. A.u University of California, USA4 aut
700a Otte, A. N.u Georgia Institute of Technology, USA4 aut
700a Pohl, M.u University of Potsdam, Germany ; DESY, Germany4 aut
700a Popkow, A.u University of California, USA4 aut
700a Prokoph, Heikeu DESY, Germany4 aut0 (Swepub:lnu)hepraa
700a Pueschel, E.u University College Dublin, Ireland4 aut
700a Quinn, J.u University College Dublin, Ireland4 aut
700a Ragan, K.u McGill University, Canada4 aut
700a Reynolds, P. T.u Cork Institute of Technology, Ireland4 aut
700a Richards, G. T.u Georgia Institute of Technology, USA4 aut
700a Roache, E.u Harvard-Smithsonian Center for Astrophysics, USA4 aut
700a Rousselle, J.u University of California, USA4 aut
700a Santander, M.u Columbia University, USA4 aut
700a Sembroski, G. H.u Purdue University, USA4 aut
700a Smith, A. W.u University of Utah, USA,Iowa State University, USA4 aut
700a Staszak, D.u McGill University, Canada4 aut
700a Telezhinsky, I.u University of Potsdam, Germany ; DESY, Germany4 aut
700a Tucci, J. V.u Purdue University, USA4 aut
700a Tyler, J.u McGill University, Canada4 aut
700a Varlotta, A.u Purdue University, USA4 aut
700a Vassiliev, V. V.u University of California, USA4 aut
700a Wakely, S. P.u University of Chicago, USA4 aut
700a Weinstein, A.u Iowa State University, USA4 aut
700a Welsing, R.u DESY, Germany4 aut
700a Williams, D. A.u University of California, USA4 aut
700a Zitzer, B.u Argonne National Laboratory, USA4 aut
710a Universitá degli Studi di Bologna, Italy ; INAF – Istituto di Radioastronomia, Italyb Pennsylvania State University, USA4 org
773t Monthly notices of the Royal Astronomical Societyd : Oxford University Pressg 446:3, s. 2456-2467q 446:3<2456-2467x 0035-8711x 1365-2966
856u https://academic.oup.com/mnras/article-pdf/446/3/2456/10447693/stu2251.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-42774
8564 8u https://doi.org/10.1093/mnras/stu2251
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-163484

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