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@ARTICLE{Abe:586997,
      author       = {Abe, H. and Abe, S. and Acciari, V. A. and Agudo, I. 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 Babic, A. and Baquero, A. and de Almeida, U.
                      Barres and Barrio, J. A. and Batkovic, I. and Baxter, J. and
                      Becerra Gonzalez, J. 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 Bonnoli, G. and Bosnjak, Z. and Burelli, I.
                      and Busetto, G. and Carosi, R. and Carretero-Castrillo, M.
                      and Castro-Tirado, A. J. 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 Do Souto Espineira,
                      E. and Dominis Prester, D. and Donini, A. and Dorner, D. and
                      Doro, M. and Elsaesser, D. and Emery, G. and Escudero, J.
                      and Fallah Ramazani, V. and Farina, L. and Fattorini, A. and
                      Foffano, L. and Font, L. and Fruck, C. and Fukami, S. and
                      Fukazawa, Y. and Lopez, R. J. Garcia and Garczarczyk, M. and
                      Gaug, M. and Paiva, J. G. Giesbrecht and Giglietto, N. and
                      Giordano, F. and Gliwny, P. and Godinovic, N. and Grau, R.
                      and Green, D. and Green, J. G. and Hadasch, D. and Hahn, A.
                      and Hassan, T. and Heckmann, L. and Herrera, J. and Hrupec,
                      D. and Hutten, M. and Imazawa, R. and Inada, T. and Iotov,
                      R. and Ishio, K. and Martınez, I. Jimenez 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 Lopez-Coto, R. and Lopez-Moya, M. and Lopez-Oramas, A.
                      and Loporchio, S. and Lorini, A. and Lyard, E. and de
                      Oliveira Fraga, B. Machado and Majumdar, P. and Makariev, M.
                      and Maneva, G. and Mang, N. and Manganaro, M. and Mangano,
                      S. and Mannheim, K. and Mariotti, M. and Martínez, M. and
                      Mas-Aguilar, A. and Mazin, D. and Menchiari, S. and Mender,
                      S. and Micanovic, 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 Okumura, A. and
                      Otero-Santos, J. and Paiano, S. and Palatiello, M. and
                      Paneque, D. and Paoletti, R. and Paredes, J. M. and
                      Pavletic, L. and Persic, M. and Pihet, M. and Pirola, G. and
                      Podobnik, F. and Prada Moroni, P. G. and Prandini, E. and
                      Principe, G. and Priyadarshi, C. and Rhode, W. and Ribo, 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 Striškovic, J. and Strom, D. and
                      Strzys, M. and Suda, Y. and Suric, T. and Tajima, H. and
                      Takahashi, M. and Takeishi, R. and Tavecchio, F. and
                      Temnikov, P. and Terauchi, K. and Terzic, T. and Teshima, M.
                      and Tosti, L. and Truzzi, S. and Tutone, A. and Ubach, S.
                      and van Scherpenberg, J. 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 Zaric, D. and Cerruti,
                      M. and Acosta-Pulido, J. A. and Lopez, R. J. Garcıa and
                      Striskovic, J. and Apolonio, G. and Bachev, R. and
                      Baloković, M. and Benítez, E. and Björklund, I. and
                      Bozhilov, V. and Brown, L. F. and Bugg, A. and Carbonell, W.
                      and Carnerero, M. I. and Carosati, D. and Casadio, C. and
                      Chamani, W. and Chen, W. P. and Chigladze, R. A. and
                      Damljanovic, G. and Epps, K. and Erkenov, A. and Feige, M.
                      and Finke, J. and Fuentes, A. and Gazeas, K. and Giroletti,
                      M. and Grishina, T. S. and Gupta, A. C. and Gurwell, , M. A.
                      and Heidemann, E. and Hiriart, D. and Hou, W. J. and
                      Hovatta, T. and Ibryamov, S. and Joner, M. D. and Gasparyan,
                      S. and Kania, J. and Kiehlmann, S. and Kimeridze, G. N. and
                      Kopatskaya, E. N. and Kopp, M. and Korte, M. and Kotas, B.
                      and Koyama, S. and Kramer, J. A. and Kunkel, L. and
                      Kurtanidze, S. O. and Kurtanidze, O. M. and Lähteenmäki,
                      A. and López, J. M. and Larionov, V. M. and Larionova, E.
                      G. and Larionova, L. V. and Leto, C. and Lorey, C. and
                      Mújica, R. and Madejski, G. M. and Marchili, N. and
                      Marscher, A. P. and Minev, M. and Modaressi, A. and
                      Morozova, D. A. and Mufakharov, T. and Myserlis, I. and
                      Nikiforova, A. A. and Nikolashvili, M. G. and Ovcharov, E.
                      and Perri, M. and Raiteri, C. M. and Readhead, A. C. S. and
                      Reimer, A. and Reinhart, D. and Righini, S. and Rosenlehner,
                      K. and Sadun, A. C. and Savchenko, S. S. and Scherbantin, A.
                      and Schneider, L. and Schoch, K. and Seifert, D. and Semkov,
                      E. and Sigua, L. A. and Singh, C. and Sola, P. and
                      Sotnikova, Y. and Spencer, M. and Steineke, R. and
                      Stojanovic, M. and Strigachev, A. and Tornikoski, M. and
                      Traianou, E. and Tramacere, A. and Troitskaya, Yu. V. and
                      Troitskiy, I. S. and Trump, J. B. and Tsai, A. and Valcheva,
                      A. and Vasilyev, A. A. and Verrecchia, F. and Villata, M.
                      and Vince, O. and Vrontaki, K. and Weaver, Z. R. and
                      Zaharieva, E. and Zottmann, N.},
      collaboration = {{MAGIC Collaboration}},
      title        = {{M}ultimessenger {C}haracterization of {M}arkarian 501
                      during {H}istorically {L}ow {X}-{R}ay and $γ$-{R}ay
                      {A}ctivity},
      reportid     = {PUBDB-2023-04081, arXiv:2210.02547},
      year         = {2023},
      note         = {55 pages, 30 figures, 14 tables, accepted by APJS.
                      Corresponding authors are L. Heckmann, D. Paneque, S.
                      Gasparyan, M. Cerruti, and N. Sahakyan},
      abstract     = {We study the broadband emission of Mrk 501 using
                      multiwavelength observations from 2017 to 2020 performed
                      with a multitude of instruments, involving, among others,
                      MAGIC, Fermi's Large Area Telescope (LAT), NuSTAR, Swift,
                      GASP-WEBT, and the Owens Valley Radio Observatory. Mrk 501
                      showed an extremely low broadband activity, which may help
                      to unravel its baseline emission. Nonetheless, significant
                      flux variations are detected at all wave bands, with the
                      highest occurring at X-rays and very-high-energy (VHE)
                      γ-rays. A significant correlation (>3σ) between X-rays and
                      VHE γ-rays is measured, supporting leptonic scenarios to
                      explain the variable parts of the emission, also during low
                      activity. This is further supported when we extend our data
                      from 2008 to 2020, and identify, for the first time,
                      significant correlations between the Swift X-Ray Telescope
                      and Fermi-LAT. We additionally find correlations between
                      high-energy γ-rays and radio, with the radio lagging by
                      more than 100 days, placing the γ-ray emission zone
                      upstream of the radio-bright regions in the jet.
                      Furthermore, Mrk 501 showed a historically low activity in
                      X-rays and VHE γ-rays from mid-2017 to mid-2019 with a
                      stable VHE flux (>0.2 TeV) of $5\%$ the emission of the Crab
                      Nebula. The broadband spectral energy distribution (SED) of
                      this 2 yr long low state, the potential baseline emission of
                      Mrk 501, can be characterized with one-zone leptonic models,
                      and with (lepto)-hadronic models fulfilling neutrino flux
                      constraints from IceCube. We explore the time evolution of
                      the SED toward the low state, revealing that the stable
                      baseline emission may be ascribed to a standing shock, and
                      the variable emission to an additional expanding or
                      traveling shock.},
      cin          = {$Z_MAGIC$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_MAGIC-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)MAGIC-20170101},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {2210.02547},
      howpublished = {arXiv:2210.02547},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2210.02547;\%\%$},
      url          = {https://bib-pubdb1.desy.de/record/586997},
}