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@ARTICLE{Acciari:599004,
      author       = {Acciari, V. A. and Aniello, T. and Ansoldi, S. and
                      Antonelli, L. A. and Engels, A. Arbet and Arcaro, C. and
                      Artero, M. and Asano, K. and Baack, D. and Babić, A. and
                      Baquero, A. and de Almeida, U. Barres and Barrio, J. A. and
                      Batković, I. and González, J. Becerra and Bednarek, W. and
                      Bernardini, E. and Bernardos, M. and Berti, A. and
                      Besenrieder, J. and Bhattacharyya, W. and Bigongiari, C. and
                      Biland, A. and Blanch, O. and Bökenkamp, H. and Bonnoli, G.
                      and Bošnjak, Ž. and Burelli, I. and Busetto, G. and
                      Carosi, R. and Carretero-Castrillo, M. and Ceribella, G. and
                      Chai, Y. and Chilingarian, A. and Cikota, S. and Colombo, E.
                      and Contreras, J. L. and Cortina, J. and Covino, S. and
                      D'Amico, G. and D'Elia, V. and Da Vela, P. and Dazzi, F. and
                      De Angelis, A. and De Lotto, B. and Del Popolo, A. and
                      Delfino, M. and Delgado, J. and Mendez, C. Delgado and
                      Depaoli, D. and Di Pierro, F. and Di Venere, L. and
                      Espiñeira, E. Do Souto and Dominis Prester, D. and Donini,
                      A. and Dorner, D. and Doro, M. and Elsaesser, D. and Emery,
                      G. and Fallah Ramazani, V. and Fariña, L. and Fattorini, A.
                      and Font, L. and Fruck, C. and Fukami, S. and Fukazawa, Y.
                      and López, R. J. García and Garczarczyk, M. and Gasparyan,
                      S. and Gaug, M. and Paiva, J. G. Giesbrecht and Giglietto,
                      N. and Giordano, F. and Gliwny, P. and Godinović, N. and
                      Green, J. G. and Green, D. and Hadasch, D. and Hahn, A. and
                      Hassan, T. and Heckmann, L. and Herrera, J. and Hrupec, D.
                      and Hütten, M. and Inada, T. and Iotov, R. and Ishio, K.
                      and Iwamura, Y. and Martínez, I. Jiménez and Jormanainen,
                      J. and Kerszberg, D. and Kobayashi, Y. and Kubo, H. and
                      Kushida, J. and Lamastra, A. and Lelas, D. and Leone, F. and
                      Lindfors, E. and Linhoff, L. and Lombardi, S. and Longo, F.
                      and López-Coto, R. and López-Moya, M. and López-Oramas,
                      A. and Loporchio, S. and Lorini, A. and Lyard, E. and Fraga,
                      B. Machado de Oliveira and Majumdar, P. and Makariev, M. and
                      Maneva, G. and Manganaro, M. and Mangano, S. and Mannheim,
                      K. and Mariotti, M. and Martínez, M. and Aguilar, A. Mas
                      and Mazin, D. and Menchiari, S. and Mender, S. and
                      Mićanović, S. and Miceli, D. and Miener, T. and Miranda,
                      J. M. and Mirzoyan, R. and Molina, E. and Mondal, H. A. and
                      Moralejo, A. and Morcuende, D. and Moreno, V. and Nakamori,
                      T. and Nanci, C. and Nava, L. and Neustroev, V. and Nievas
                      Rosillo, M. and Nigro, C. and Nilsson, K. and Nishijima, K.
                      and Ekoume, T. Njoh and Noda, K. and Nozaki, S. and Ohtani,
                      Y. and Oka, T. and Otero-Santos, J. and Paiano, S. and
                      Palatiello, M. and Paneque, D. and Paoletti, R. and Paredes,
                      J. M. and Pavletić, L. and Persic, M. and Pihet, M. and
                      Podobnik, F. and Prada Moroni, P. G. and Prandini, E. and
                      Principe, G. and Priyadarshi, C. and Puljak, I. and Rhode,
                      W. and Ribó, M. and Rico, J. and Righi, C. and Rugliancich,
                      A. and Sahakyan, N. and Saito, T. and Sakurai, S. and
                      Satalecka, K. and Saturni, F. G. and Schleicher, B. and
                      Schmidt, K. and Schmuckermaier, F. and Schubert, J. L. and
                      Schweizer, T. and Sitarek, J. and Sliusar, V. and
                      Sobczynska, D. and Spolon, A. and Stamerra, A. and
                      Strišković, J. and Strom, D. and Strzys, M. and Suda, Y.
                      and Surić, T. and Takahashi, M. and Takeishi, R. and
                      Tavecchio, F. and Temnikov, P. and Terzić, T. and Teshima,
                      M. and Tosti, L. and Truzzi, S. and Tutone, A. and Ubach, S.
                      and van Scherpenberg, J. and Vanzo, G. and Vazquez Acosta,
                      M. and Ventura, S. and Verguilov, V. and Viale, I. and
                      Vigorito, C. F. and Vitale, V. and Vovk, I. and Walter, R.
                      and Will, M. and Wunderlich, C. and Yamamoto, T. and Zarić,
                      D. and Acosta-Pulido, J. A. and D'Ammando, F. and Hovatta,
                      T. and Kiehlmann, S. and Liodakis, I. and Leto, C. and
                      Max-Moerbeck, W. and Pacciani, L. and Perri, M. and
                      Readhead, A. C. S. and Reeves, R. A. and Verrecchia, F.},
      collaboration = {{MAGIC Collaboration}},
      title        = {{L}ong-term multi-wavelength study of 1{ES} 0647+250},
      journal      = {Astronomy and astrophysics},
      volume       = {670},
      issn         = {0004-6361},
      address      = {Les Ulis},
      publisher    = {EDP Sciences},
      reportid     = {PUBDB-2023-07088, arXiv:2211.13268},
      pages        = {A49},
      year         = {2023},
      note         = {$A\&A$ 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)},
      abstract     = {The 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.},
      keywords     = {blazar: emission (INSPIRE) / model: leptonic (INSPIRE) /
                      spectral (INSPIRE) / MAGIC (INSPIRE) / GeV (INSPIRE) / flux
                      (INSPIRE) / redshift (INSPIRE) / gamma ray: VHE (INSPIRE) /
                      gamma ray: energy spectrum (INSPIRE) / correlation function
                      (INSPIRE) / correlation (INSPIRE) / TeV (INSPIRE) / GLAST
                      (INSPIRE) / fractional (INSPIRE) / X-ray (INSPIRE)},
      cin          = {$Z_CTAS$ / $Z_MAGIC$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_CTAS-20210408$ /
                      $I:(DE-H253)Z_MAGIC-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)CTA-20150101 / EXP:(DE-H253)MAGIC-20170101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2211.13268},
      howpublished = {arXiv:2211.13268},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2211.13268;\%\%$},
      UT           = {WOS:001006118000002},
      doi          = {10.1051/0004-6361/202244477},
      url          = {https://bib-pubdb1.desy.de/record/599004},
}