% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @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}, }