000293214 001__ 293214
000293214 005__ 20250730113838.0
000293214 0247_ $$2doi$$a10.1088/0004-637X/802/1/65
000293214 0247_ $$2ISSN$$a0004-637X
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000293214 0247_ $$2ISSN$$a1538-4357
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000293214 0247_ $$2datacite_doi$$a10.3204/PUBDB-2016-00370
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000293214 037__ $$aPUBDB-2016-00370
000293214 082__ $$a520
000293214 1001_ $$aAbramowski, A.$$b0
000293214 245__ $$aThe 2012 Flare of PG 1553+113 Seen with H.E.S.S. and Fermi -Lat
000293214 260__ $$aChicago, Ill. [u.a.]$$bUniv.11032$$c2015
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000293214 500__ $$a(c) The American Astronomical Society
000293214 520__ $$aVery high energy (VHE, E > 100 GeV) $\gamma-ray$ flaring activity of the high-frequency peaked BL Lac object PG 1553+113 has been detected by the H.E.S.S. telescopes. The flux of the source increased by a factor of 3 during the nights of 2012 April 26 and 27 with respect to the archival measurements with a hint of intra-night variability. No counterpart of this event has been detected in the Fermi-Large Area Telescope data. This pattern is consistent with VHE $\gamma-ray$ flaring being caused by the injection of ultrarelativistic particles, emitting $\gamma-rays$ at the highest energies. The dataset offers a unique opportunity to constrain the redshift of this source at z = 0.49 $\pm$ 0.04 using a novel method based on Bayesian statistics. The indication of intra-night variability is used to introduce a novel method to probe for a possible Lorentz invariance violation (LIV), and to set limits on the energy scale at which Quantum Gravity (QG) effects causing LIV may arise. For the subluminal case, the derived limits are $E_{QG,1}$ > 4.10 × $10^{17}$ GeV and $E_{QG,2}$ > 2.10 × $10^{10}$ GeV for linear and quadratic LIV effects, respectively.
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000293214 536__ $$0G:(EU-Grant)259391$$aP-WIND - New light on the gamma-ray sky: unveiling cosmic-ray accelerators in the Milky Way and their relation to pulsar wind nebulae (259391)$$c259391$$fERC-2010-StG_20091028$$x1
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000293214 7001_ $$aAharonian, F.$$b1
000293214 7001_ $$aBenkhali, F. Ait$$b2
000293214 7001_ $$aAkhperjanian, A. G.$$b3
000293214 7001_ $$aAngüner, E. O.$$b4
000293214 7001_ $$aBackes, M.$$b5
000293214 7001_ $$aBalenderan, S.$$b6
000293214 7001_ $$aBalzer, A.$$b7
000293214 7001_ $$aBarnacka, A.$$b8
000293214 7001_ $$aBecherini, Y.$$b9
000293214 7001_ $$aTjus, J. Becker$$b10
000293214 7001_ $$aBerge, D.$$b11
000293214 7001_ $$aBernhard, S.$$b12
000293214 7001_ $$aBernlöhr, K.$$b13
000293214 7001_ $$aBirsin, E.$$b14
000293214 7001_ $$aBiteau, J.$$b15
000293214 7001_ $$aBöttcher, M.$$b16
000293214 7001_ $$aBoisson, C.$$b17
000293214 7001_ $$aBolmont, J.$$b18
000293214 7001_ $$aBordas, P.$$b19
000293214 7001_ $$aBregeon, J.$$b20
000293214 7001_ $$0P:(DE-HGF)0$$aBrun, F.$$b21$$eCorresponding author
000293214 7001_ $$aBrun, P.$$b22
000293214 7001_ $$aBryan, M.$$b23
000293214 7001_ $$aBulik, T.$$b24
000293214 7001_ $$aCarrigan, S.$$b25
000293214 7001_ $$aCasanova, S.$$b26
000293214 7001_ $$aChadwick, P. M.$$b27
000293214 7001_ $$aChakraborty, N.$$b28
000293214 7001_ $$aChalme-Calvet, R.$$b29
000293214 7001_ $$aChaves, R. C. G.$$b30
000293214 7001_ $$aChrétien, M.$$b31
000293214 7001_ $$aColafrancesco, S.$$b32
000293214 7001_ $$aCologna, G.$$b33
000293214 7001_ $$aConrad, J.$$b34
000293214 7001_ $$0P:(DE-HGF)0$$aCouturier, C.$$b35$$eCorresponding author
000293214 7001_ $$aCui, Y.$$b36
000293214 7001_ $$aDalton, M.$$b37
000293214 7001_ $$aDavids, I. D.$$b38
000293214 7001_ $$aDegrange, B.$$b39
000293214 7001_ $$aDeil, C.$$b40
000293214 7001_ $$adeWilt, P.$$b41
000293214 7001_ $$aDjannati-Ataï, A.$$b42
000293214 7001_ $$aDomainko, W.$$b43
000293214 7001_ $$aDonath, A.$$b44
000293214 7001_ $$aDrury, L. O’C.$$b45
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000293214 7001_ $$aEgberts, K.$$b51
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000293214 7001_ $$aFeinstein, F.$$b56
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000293214 7001_ $$aGrudzińska, M.$$b72
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000293214 7001_ $$aIvascenko, A.$$b87
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000293214 7001_ $$aJahn, C.$$b89
000293214 7001_ $$aJamrozy, M.$$b90
000293214 7001_ $$aJaniak, M.$$b91
000293214 7001_ $$aJankowsky, F.$$b92
000293214 7001_ $$aJung, I.$$b93
000293214 7001_ $$aKastendieck, M. A.$$b94
000293214 7001_ $$aKatarzyński, K.$$b95
000293214 7001_ $$aKatz, U.$$b96
000293214 7001_ $$aKaufmann, S.$$b97
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000293214 7001_ $$aLemoine-Goumard, M.$$b114
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000293214 7001_ $$aMeintjes, P. J.$$b127
000293214 7001_ $$aMenzler, U.$$b128
000293214 7001_ $$aMeyer, M.$$b129
000293214 7001_ $$aMitchell, A. M. W.$$b130
000293214 7001_ $$aModerski, R.$$b131
000293214 7001_ $$aMohamed, M.$$b132
000293214 7001_ $$aMorå, K.$$b133
000293214 7001_ $$aMoulin, E.$$b134
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000293214 7001_ $$aNaurois, M. de$$b136
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000293214 7001_ $$aOdaka, H.$$b140
000293214 7001_ $$aOhm, S.$$b141
000293214 7001_ $$aOpitz, B.$$b142
000293214 7001_ $$aOstrowski, M.$$b143
000293214 7001_ $$aOya, I.$$b144
000293214 7001_ $$aPanter, M.$$b145
000293214 7001_ $$aParsons, R. D.$$b146
000293214 7001_ $$aPaz Arribas, M.$$b147
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000293214 7001_ $$aPelletier, G.$$b149
000293214 7001_ $$aPerez, J.$$b150
000293214 7001_ $$aPetrucci, P.-O.$$b151
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000293214 7001_ $$aPoon, H.$$b154
000293214 7001_ $$aPühlhofer, G.$$b155
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000293214 7001_ $$ade los Reyes, R.$$b163
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000293214 7001_ $$aSalek, D.$$b172
000293214 7001_ $$0P:(DE-HGF)0$$aSanchez, D. A.$$b173$$eCorresponding author
000293214 7001_ $$aSantangelo, A.$$b174
000293214 7001_ $$aSchlickeiser, R.$$b175
000293214 7001_ $$aSchüssler, F.$$b176
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000293214 7001_ $$aValerius, K.$$b197
000293214 7001_ $$avan Eldik, C.$$b198
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000293214 7001_ $$aZechlin, H.-S.$$b226
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