000293264 001__ 293264
000293264 005__ 20250730113847.0
000293264 0247_ $$2doi$$a10.1093/mnras/stu2251
000293264 0247_ $$2ISSN$$a0035-8711
000293264 0247_ $$2ISSN$$a1365-2966
000293264 0247_ $$2WOS$$aWOS:000350272300020
000293264 0247_ $$2datacite_doi$$a10.3204/PUBDB-2016-00419
000293264 0247_ $$2inspire$$ainspire:1324339
000293264 0247_ $$2altmetric$$aaltmetric:2814598
000293264 0247_ $$2arXiv$$aarXiv:1410.7144
000293264 0247_ $$2openalex$$aopenalex:W2017492270
000293264 037__ $$aPUBDB-2016-00419
000293264 082__ $$a520
000293264 088__ $$2arXiv$$aarXiv:1410.7144
000293264 1001_ $$0P:(DE-HGF)0$$aD'Ammando, F.$$b0$$eCorresponding author
000293264 245__ $$aThe most powerful flaring activity from the NLSy1 PMN J0948+0022
000293264 260__ $$aOxford$$bOxford Univ. Press$$c2015
000293264 3367_ $$2DRIVER$$aarticle
000293264 3367_ $$2DataCite$$aOutput Types/Journal article
000293264 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1598607757_15986
000293264 3367_ $$2BibTeX$$aARTICLE
000293264 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000293264 3367_ $$00$$2EndNote$$aJournal Article
000293264 500__ $$a(c) The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
000293264 520__ $$aWe report on multifrequency observations performed during 2012 December–2013 August of the first narrow-line Seyfert 1 galaxy detected in $\gamma$-rays, PMN J0948+0022 (z = 0.5846). A γ-ray flare was observed by the Large Area Telescope on board Fermi during 2012 December–2013 January, reaching a daily peak flux in the 0.1–100 GeV energy range of (155 $\pm$ 31) × $10^{−8}$ ph $cm^{−2} s^{−1}$ on 2013 January 1, corresponding to an apparent isotropic luminosity of $\sim$ 1.5 × $10^{48}$ erg $s^{−1}$. The $\gamma$-ray flaring period triggered Swift and Very Energetic Radiation Imaging Telescope Array System (VERITAS) observations in addition to radio and optical monitoring by Owens Valley Radio Observatory, Monitoring Of Jets in Active galactic nuclei with VLBA Experiments, and Catalina Real-time Transient Survey. A strong flare was observed in optical, UV, and X-rays on 2012 December 30, quasi-simultaneously to the $\gamma$-ray flare, reaching a record flux for this source from optical to $\gamma$-rays. VERITAS observations at very high energy (E > 100 GeV) during 2013 January 6–17 resulted in an upper limit of $F_{>0.2 TeV}$ < 4.0 × $10^{−12} ph cm^{−2} s^{−1}$. We compared the spectral energy distribution (SED) of the flaring state in 2013 January with that of an intermediate state observed in 2011. The two SEDs, modelled as synchrotron emission and an external Compton scattering of seed photons from a dust torus, can be modelled by changing both the electron distribution parameters and the magnetic field.
000293264 536__ $$0G:(DE-HGF)POF2-523$$a523 - High-energy gamma ray astronomy (POF2-523)$$cPOF2-523$$fPOF II$$x0
000293264 588__ $$aDataset connected to CrossRef
000293264 693__ $$0EXP:(DE-MLZ)External-20140101$$5EXP:(DE-MLZ)External-20140101$$eMeasurement at external facility$$x0
000293264 7001_ $$aOrienti, M.$$b1
000293264 7001_ $$aFinke, J.$$b2
000293264 7001_ $$aRaiteri, C. M.$$b3
000293264 7001_ $$aHovatta, T.$$b4
000293264 7001_ $$aLarsson, J.$$b5
000293264 7001_ $$aMax-Moerbeck, W.$$b6
000293264 7001_ $$aPerkins, J.$$b7
000293264 7001_ $$aReadhead, A. C. S.$$b8
000293264 7001_ $$aRichards, J. L.$$b9
000293264 7001_ $$aBeilicke, M.$$b10
000293264 7001_ $$aBenbow, W.$$b11
000293264 7001_ $$aBerger, K.$$b12
000293264 7001_ $$aBird, R.$$b13
000293264 7001_ $$aBugaev, V.$$b14
000293264 7001_ $$aCardenzana, J. V.$$b15
000293264 7001_ $$aCerruti, M.$$b16
000293264 7001_ $$0P:(DE-H253)PIP1018140$$aChen, Xuhui$$b17$$udesy
000293264 7001_ $$aCiupik, L.$$b18
000293264 7001_ $$aDickinson, H. J.$$b19
000293264 7001_ $$aEisch, J. D.$$b20
000293264 7001_ $$aErrando, M.$$b21
000293264 7001_ $$aFalcone, A.$$b22
000293264 7001_ $$aFinley, J. P.$$b23
000293264 7001_ $$0P:(DE-H253)PIP1018032$$aFleischhack, H.$$b24$$udesy
000293264 7001_ $$aFortin, P.$$b25
000293264 7001_ $$aFortson, L.$$b26
000293264 7001_ $$aFurniss, A.$$b27
000293264 7001_ $$aGerard, L.$$b28
000293264 7001_ $$aGillanders, G. H.$$b29
000293264 7001_ $$aGriffiths, S. T.$$b30
000293264 7001_ $$aGrube, J.$$b31
000293264 7001_ $$aGyuk, G.$$b32
000293264 7001_ $$aHakansson, N.$$b33
000293264 7001_ $$aHolder, J.$$b34
000293264 7001_ $$aHumensky, T. B.$$b35
000293264 7001_ $$aKar, P.$$b36
000293264 7001_ $$aKertzman, M.$$b37
000293264 7001_ $$aKhassen, Y.$$b38
000293264 7001_ $$aKieda, D.$$b39
000293264 7001_ $$aKrennrich, F.$$b40
000293264 7001_ $$aKumar, S.$$b41
000293264 7001_ $$aLang, M. J.$$b42
000293264 7001_ $$0P:(DE-H253)PIP1011664$$aMaier, G.$$b43$$udesy
000293264 7001_ $$aMcCann, A.$$b44
000293264 7001_ $$aMeagher, K.$$b45
000293264 7001_ $$aMoriarty, P.$$b46
000293264 7001_ $$aMukherjee, R.$$b47
000293264 7001_ $$aNieto, D.$$b48
000293264 7001_ $$0P:(DE-HGF)0$$ade Bhroithe, A. O.$$b49
000293264 7001_ $$aOng, R. A.$$b50
000293264 7001_ $$aOtte, A. N.$$b51
000293264 7001_ $$0P:(DE-H253)PIP1010085$$aPohl, Martin$$b52$$udesy
000293264 7001_ $$aPopkow, A.$$b53
000293264 7001_ $$0P:(DE-H253)PIP1006678$$aProkoph, H.$$b54$$udesy
000293264 7001_ $$aPueschel, E.$$b55
000293264 7001_ $$aQuinn, J.$$b56
000293264 7001_ $$aRagan, K.$$b57
000293264 7001_ $$aReynolds, P. T.$$b58
000293264 7001_ $$aRichards, G. T.$$b59
000293264 7001_ $$aRoache, E.$$b60
000293264 7001_ $$aRousselle, J.$$b61
000293264 7001_ $$aSantander, M.$$b62
000293264 7001_ $$aSembroski, G. H.$$b63
000293264 7001_ $$aSmith, A. W.$$b64
000293264 7001_ $$aStaszak, D.$$b65
000293264 7001_ $$aTelezhinsky, I.$$b66
000293264 7001_ $$aTucci, J. V.$$b67
000293264 7001_ $$aTyler, J.$$b68
000293264 7001_ $$aVarlotta, A.$$b69
000293264 7001_ $$aVassiliev, V. V.$$b70
000293264 7001_ $$aWakely, S. P.$$b71
000293264 7001_ $$aWeinstein, A.$$b72
000293264 7001_ $$0P:(DE-H253)PIP1006926$$aWelsing, R.$$b73$$udesy
000293264 7001_ $$aWilliams, D. A.$$b74
000293264 7001_ $$aZitzer, B.$$b75
000293264 773__ $$0PERI:(DE-600)2016084-7$$a10.1093/mnras/stu2251$$gVol. 446, no. 3, p. 2456 - 2467$$n3$$p2456 - 2467$$tMonthly notices of the Royal Astronomical Society$$v446$$x1365-2966$$y2015
000293264 7870_ $$0PUBDB-2014-04309$$aD'Ammando, F. et.al.$$d2014$$iIsParent$$rarXiv:1410.7144$$tThe most powerful flaring activity from the NLSy1 PMN J0948+0022
000293264 8564_ $$uhttps://bib-pubdb1.desy.de/record/293264/files/MNRAS-2015-D%27Ammando-2456-67.pdf$$yOpenAccess
000293264 8564_ $$uhttps://bib-pubdb1.desy.de/record/293264/files/MNRAS-2015-D%27Ammando-2456-67.gif?subformat=icon$$xicon$$yOpenAccess
000293264 8564_ $$uhttps://bib-pubdb1.desy.de/record/293264/files/MNRAS-2015-D%27Ammando-2456-67.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000293264 8564_ $$uhttps://bib-pubdb1.desy.de/record/293264/files/MNRAS-2015-D%27Ammando-2456-67.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000293264 8564_ $$uhttps://bib-pubdb1.desy.de/record/293264/files/MNRAS-2015-D%27Ammando-2456-67.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000293264 8564_ $$uhttps://bib-pubdb1.desy.de/record/293264/files/MNRAS-2015-D%27Ammando-2456-67.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000293264 909CO $$ooai:bib-pubdb1.desy.de:293264$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000293264 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1018140$$aDeutsches Elektronen-Synchrotron$$b17$$kDESY
000293264 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1018032$$aDeutsches Elektronen-Synchrotron$$b24$$kDESY
000293264 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1011664$$aDeutsches Elektronen-Synchrotron$$b43$$kDESY
000293264 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-HGF)0$$aDeutsches Elektronen-Synchrotron$$b49$$kDESY
000293264 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1010085$$aDeutsches Elektronen-Synchrotron$$b52$$kDESY
000293264 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1006678$$aDeutsches Elektronen-Synchrotron$$b54$$kDESY
000293264 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1006926$$aDeutsches Elektronen-Synchrotron$$b73$$kDESY
000293264 9132_ $$0G:(DE-HGF)POF3-613$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vMatter and Radiation from the Universe$$x0
000293264 9131_ $$0G:(DE-HGF)POF2-523$$1G:(DE-HGF)POF2-520$$2G:(DE-HGF)POF2-500$$3G:(DE-HGF)POF2$$4G:(DE-HGF)POF$$aDE-HGF$$bStruktur der Materie$$lAstroteilchenphysik$$vHigh-energy gamma ray astronomy$$x1
000293264 9141_ $$y2015
000293264 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000293264 915__ $$0LIC:(DE-HGF)PublisherOA$$2HGFVOC$$aFree to read
000293264 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bMON NOT R ASTRON SOC : 2014
000293264 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences
000293264 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection
000293264 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index
000293264 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded
000293264 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000293264 915__ $$0StatID:(DE-HGF)9905$$2StatID$$aIF >= 5$$bMON NOT R ASTRON SOC : 2014
000293264 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline
000293264 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz
000293264 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bThomson Reuters Master Journal List
000293264 9201_ $$0I:(DE-H253)ZEU-EXP_AT-20120731$$kZEU-EXP/AT$$lAstroteilchenphysik$$x0
000293264 980__ $$ajournal
000293264 980__ $$aVDB
000293264 980__ $$aUNRESTRICTED
000293264 980__ $$aI:(DE-H253)ZEU-EXP_AT-20120731
000293264 9801_ $$aFullTexts