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000599004 0247_ $$2ISSN$$a1432-0746
000599004 0247_ $$2arXiv$$aarXiv:2211.13268
000599004 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-07088
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000599004 041__ $$aEnglish
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000599004 088__ $$2arXiv$$aarXiv:2211.13268
000599004 1001_ $$aAcciari, V. A.$$b0
000599004 245__ $$aLong-term multi-wavelength study of 1ES 0647+250
000599004 260__ $$aLes Ulis$$bEDP Sciences$$c2023
000599004 3367_ $$2DRIVER$$aarticle
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000599004 500__ $$aA&A 670, A49 (2023). 20 pages, 7 figures. Accepted in A&A. Corresponding authors: Jorge Otero-Santos; Daniel Morcuende; Vandad Fallah Ramazani; Daniela Dorner; David Paneque (mailto: contact.magic@mpp.mpg.de)
000599004 520__ $$aThe BL Lac object 1ES 0647+250 is one of the few distant $\gamma$-ray emitting blazars detected at very high energies (VHE, $\gtrsim$100 GeV) during a non-flaring state. It was detected with the MAGIC telescopes during its low activity in the years 2009-2011, as well as during three flaring activities in the years 2014, 2019 and 2020, with the highest VHE flux in the latter epoch. An extensive multi-instrument data set was collected within several coordinated observing campaigns throughout these years. We aim to characterise the long-term multi-band flux variability of 1ES 0647+250, as well as its broadband spectral energy distribution (SED) during four distinct activity states selected in four different epochs, in order to constrain the physical parameters of the blazar emission region under certain assumptions. We evaluate the variability and correlation of the emission in the different energy bands with the fractional variability and the Z-transformed Discrete Correlation Function, as well as its spectral evolution in X-rays and $\gamma$ rays. Owing to the controversy in the redshift measurements of 1ES 0647+250 reported in the literature, we also estimate its distance in an indirect manner through the comparison of the GeV and TeV spectra from simultaneous observations with Fermi-LAT and MAGIC during the strongest flaring activity detected to date. Moreover, we interpret the SEDs from the four distinct activity states within the framework of one-component and two-component leptonic models, proposing specific scenarios that are able to reproduce the available multi-instrument data.
000599004 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
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000599004 650_7 $$2INSPIRE$$ablazar: emission
000599004 650_7 $$2INSPIRE$$amodel: leptonic
000599004 650_7 $$2INSPIRE$$aspectral
000599004 650_7 $$2INSPIRE$$aMAGIC
000599004 650_7 $$2INSPIRE$$aGeV
000599004 650_7 $$2INSPIRE$$aflux
000599004 650_7 $$2INSPIRE$$aredshift
000599004 650_7 $$2INSPIRE$$agamma ray: VHE
000599004 650_7 $$2INSPIRE$$agamma ray: energy spectrum
000599004 650_7 $$2INSPIRE$$acorrelation function
000599004 650_7 $$2INSPIRE$$acorrelation
000599004 650_7 $$2INSPIRE$$aTeV
000599004 650_7 $$2INSPIRE$$aGLAST
000599004 650_7 $$2INSPIRE$$afractional
000599004 650_7 $$2INSPIRE$$aX-ray
000599004 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
000599004 693__ $$0EXP:(DE-H253)MAGIC-20170101$$5EXP:(DE-H253)MAGIC-20170101$$eMajor Atmospheric Gamma Imaging Cherenkov$$x1
000599004 7001_ $$aAniello, T.$$b1
000599004 7001_ $$aAnsoldi, S.$$b2
000599004 7001_ $$aAntonelli, L. A.$$b3
000599004 7001_ $$aEngels, A. Arbet$$b4
000599004 7001_ $$aArcaro, C.$$b5
000599004 7001_ $$aArtero, M.$$b6
000599004 7001_ $$aAsano, K.$$b7
000599004 7001_ $$aBaack, D.$$b8
000599004 7001_ $$0P:(DE-H253)PIP1102839$$aBabić, A.$$b9
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000599004 7001_ $$ade Almeida, U. Barres$$b11
000599004 7001_ $$aBarrio, J. A.$$b12
000599004 7001_ $$aBatković, I.$$b13
000599004 7001_ $$aGonzález, J. Becerra$$b14
000599004 7001_ $$aBednarek, W.$$b15
000599004 7001_ $$aBernardini, E.$$b16
000599004 7001_ $$aBernardos, M.$$b17
000599004 7001_ $$aBerti, A.$$b18
000599004 7001_ $$aBesenrieder, J.$$b19
000599004 7001_ $$0P:(DE-H253)PIP1028466$$aBhattacharyya, W.$$b20
000599004 7001_ $$aBigongiari, C.$$b21
000599004 7001_ $$aBiland, A.$$b22
000599004 7001_ $$aBlanch, O.$$b23
000599004 7001_ $$aBökenkamp, H.$$b24
000599004 7001_ $$aBonnoli, G.$$b25
000599004 7001_ $$aBošnjak, Ž.$$b26
000599004 7001_ $$aBurelli, I.$$b27
000599004 7001_ $$aBusetto, G.$$b28
000599004 7001_ $$aCarosi, R.$$b29
000599004 7001_ $$aCarretero-Castrillo, M.$$b30
000599004 7001_ $$aCeribella, G.$$b31
000599004 7001_ $$aChai, Y.$$b32
000599004 7001_ $$aChilingarian, A.$$b33
000599004 7001_ $$aCikota, S.$$b34
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000599004 7001_ $$aD'Amico, G.$$b39
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000599004 7001_ $$aEspiñeira, E. Do Souto$$b52
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000599004 7001_ $$aDonini, A.$$b54
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000599004 7001_ $$aDoro, M.$$b56
000599004 7001_ $$aElsaesser, D.$$b57
000599004 7001_ $$aEmery, G.$$b58
000599004 7001_ $$aFallah Ramazani, V.$$b59
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000599004 7001_ $$aGodinović, N.$$b74
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000599004 7001_ $$aLoporchio, S.$$b104
000599004 7001_ $$aLorini, A.$$b105
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000599004 7001_ $$aMannheim, K.$$b113
000599004 7001_ $$aMariotti, M.$$b114
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000599004 7001_ $$aAguilar, A. Mas$$b116
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000599004 7001_ $$aMenchiari, S.$$b118
000599004 7001_ $$aMender, S.$$b119
000599004 7001_ $$aMićanović, S.$$b120
000599004 7001_ $$aMiceli, D.$$b121
000599004 7001_ $$aMiener, T.$$b122
000599004 7001_ $$aMiranda, J. M.$$b123
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000599004 7001_ $$aMondal, H. A.$$b126
000599004 7001_ $$aMoralejo, A.$$b127
000599004 7001_ $$0P:(DE-H253)PIP1080676$$aMorcuende, D.$$b128$$eCorresponding author
000599004 7001_ $$0P:(DE-H253)PIP1017164$$aMoreno, V.$$b129
000599004 7001_ $$aNakamori, T.$$b130
000599004 7001_ $$aNanci, C.$$b131
000599004 7001_ $$aNava, L.$$b132
000599004 7001_ $$aNeustroev, V.$$b133
000599004 7001_ $$aNievas Rosillo, M.$$b134
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000599004 7001_ $$aNishijima, K.$$b137
000599004 7001_ $$aEkoume, T. Njoh$$b138
000599004 7001_ $$aNoda, K.$$b139
000599004 7001_ $$aNozaki, S.$$b140
000599004 7001_ $$aOhtani, Y.$$b141
000599004 7001_ $$aOka, T.$$b142
000599004 7001_ $$0P:(DE-HGF)0$$aOtero-Santos, J.$$b143$$eCorresponding author
000599004 7001_ $$aPaiano, S.$$b144
000599004 7001_ $$aPalatiello, M.$$b145
000599004 7001_ $$0P:(DE-HGF)0$$aPaneque, D.$$b146$$eCorresponding author
000599004 7001_ $$0P:(DE-H253)PIP1026960$$aPaoletti, R.$$b147
000599004 7001_ $$aParedes, J. M.$$b148
000599004 7001_ $$aPavletić, L.$$b149
000599004 7001_ $$aPersic, M.$$b150
000599004 7001_ $$aPihet, M.$$b151
000599004 7001_ $$aPodobnik, F.$$b152
000599004 7001_ $$aPrada Moroni, P. G.$$b153
000599004 7001_ $$aPrandini, E.$$b154
000599004 7001_ $$aPrincipe, G.$$b155
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000599004 7001_ $$aViale, I.$$b198
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