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@ARTICLE{Abe:623126,
      author       = {Abe, S. and Abhir, J. and Abhishek, A. and Acciari, V. A.
                      and Aguasca-Cabot, A. and Agudo, I. and Aniello, T. and
                      Ansoldi, S. and Antonelli, L. A. and Arbet Engels, A. and
                      Arcaro, C. and Artero, M. and Asano, K. and Babić, A. and
                      Baquero, A. and Barres de Almeida, U. and Barrio, J. A. and
                      Batković, I. and Bautista, A. and Baxter, J. and Becerra
                      González, J. and Bednarek, W. and Bernardini, E. and
                      Bernete, J. and Berti, A. and Besenrieder, J. and
                      Bigongiari, C. and Biland, A. and Blanch, O. and Bonnoli, G.
                      and Bošnjak, Ž and Bronzini, E. and Burelli, I. and
                      Busetto, G. and Campoy-Ordaz, A. and Carosi, A. and Carosi,
                      R. and Carretero-Castrillo, M. and Castro-Tirado, A. J. and
                      Cerasole, D. and Ceribella, G. and Chai, Y. and Cifuentes,
                      A. and Colombo, E. and Contreras, J. L. and Cortina, J. and
                      Covino, S. and D’Amico, G. and D’Ammando, F. and
                      D’Elia, V. and Da Vela, P. and Dazzi, F. and De Angelis,
                      A. and De Lotto, B. and de Menezes, R. and Del Popolo, A.
                      and Delfino, M. and Delgado, J. and Delgado Mendez, C. and
                      Di Pierro, F. and Di Tria, R. and Di Venere, L. and Dominis
                      Prester, D. and Donini, A. and Dorner, D. and Doro, M. and
                      Elsaesser, D. and Emery, G. and Escudero, J. and Fariña, L.
                      and Fattorini, A. and Foffano, L. and Font, L. and Fröse,
                      S. and Fukami, S. and Fukazawa, Y. and García López, R. J.
                      and Garczarczyk, M. and Gasparyan, S. and Gaug, M. and
                      Giesbrecht Paiva, J. G. and Giglietto, N. and Giordano, F.
                      and Gliwny, P. and Godinović, N. and Gradetzke, T. and
                      Grau, R. and Green, D. and Green, J. G. and Günther, P. and
                      Hadasch, D. and Hahn, A. and Hassan, T. and Heckmann, L. and
                      Herrera, J. and Hrupec, D. and Hütten, M. and Imazawa, R.
                      and Ishio, K. and Jiménez Martínez, I. and Jormanainen, J.
                      and Kayanoki, T. and Kerszberg, D. and Kobayashi, Y. and
                      Kouch, P. M. and Kubo, H. and Kushida, J. and Láinez, M.
                      and Lamastra, A. 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 Machado de Oliveira Fraga, B.
                      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 Martínez-Chicharro, M.
                      and Mas-Aguilar, A. and Mazin, D. and Menchiari, S. and
                      Mender, S. and Miceli, D. and Miener, T. and Miranda, J. M.
                      and Mirzoyan, R. and Molero González, M. and Molina, E. and
                      Mondal, H. A. and Moralejo, A. and Morcuende, D. and
                      Nakamori, T. and Nanci, C. and Neustroev, V. and Nickel, L.
                      and Nievas Rosillo, M. and Nigro, C. and Nikolić, L. and
                      Nilsson, K. and Nishijima, K. and Njoh Ekoume, T. and Noda,
                      K. and Nozaki, S. and Ohtani, Y. and Okumura, A. and
                      Otero-Santos, J. and Paiano, S. and Palatiello, M. and
                      Paneque, D. and Paoletti, R. and Paredes, J. M. and
                      Peresano, M. 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 Ribó, M.
                      and Rico, J. and Righi, C. and Sahakyan, N. and Saito, T.
                      and Satalecka, K. and Saturni, F. G. and Schleicher, B. and
                      Schmidt, K. and Schmuckermaier, F. and Schubert, J. L. and
                      Schweizer, T. and Sciaccaluga, A. and Silvestri, G. 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 Suutarinen, S. and Tajima, H.
                      and Takahashi, M. and Takeishi, R. and Temnikov, P. and
                      Terauchi, K. and Terzić, T. and Teshima, M. and Truzzi, S.
                      and Tutone, A. and Ubach, S. and van Scherpenberg, J. and
                      Vazquez Acosta, M. and Ventura, S. 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
                      Zywucka, N. and Ramazani, V. F. and Buson, S. and Ciprini,
                      S.},
      collaboration = {{Magic Collaboration}},
      title        = {{C}onstraints on {VHE} gamma-ray emission of flat spectrum
                      radio quasars with the {MAGIC} telescopes},
      journal      = {Monthly notices of the Royal Astronomical Society},
      volume       = {535},
      number       = {2},
      issn         = {0035-8711},
      address      = {Oxford},
      publisher    = {Oxford Univ. Press},
      reportid     = {PUBDB-2025-00613, arXiv:2403.13713},
      series       = {2682130},
      pages        = {1484 - 1506},
      year         = {2024},
      note         = {DFG Grant 1491; DFG Grant BU 3832/2-1},
      abstract     = {Blazars are a class of active galactic nuclei (AGN) where
                      the relativistic jet is pointed towards the observer. They
                      are powerful sources of non-thermal radiation from radio to
                      Very high energy(VHE) gamma-rays. Flat Spectrum Radio
                      Quasars (FSRQs) are a subclass of blazars where there are
                      broad absorption or emission lines present in the optical
                      spectra.The observed properties of FSRQs are strongly
                      affected by the magnetic field in the accretion disk which
                      changes the UV emission of Broad Line Region (BLR) and
                      infrared emission from the Dusty Torus.While many (774 as
                      reported in 4FGL-DR2 catalogue) FSRQs have been detected at
                      high energies(E>100 MeV), only a few (9 as of now) could be
                      detected at very-high energies (> 100 GeV).In this work, we
                      present observations of nine FSRQs performed by MAGIC
                      between 2008 and 2020 with a total observation time being
                      174 hours. For two of the sources, CTA102 and B2 2234+28A,
                      we include observations from the Fermi-LAT, Swift-UVOT,
                      Swift-XRT and KVA (Kungliga Vetenskapsakademien). The
                      multi-wavelength spectra for these sources show hints of
                      absorption.We also modelled the broadband emission of the
                      sources to look for signatures of absorption of VHE
                      gamma-ray emission in the BLR region.},
      month         = {Jul},
      date          = {2023-07-26},
      organization  = {38th International Cosmic Ray
                       Conference, Nagoya (Japan), 26 Jul 2023
                       - 3 Aug 2023},
      keywords     = {gamma ray: VHE (INSPIRE) / gamma ray: emission (INSPIRE) /
                      energy: high (INSPIRE) / jet: relativistic (INSPIRE) /
                      absorption (INSPIRE) / AGN (INSPIRE) / MAGIC (INSPIRE) /
                      blazar (INSPIRE) / quasar (INSPIRE) / GeV (INSPIRE) / torus
                      (INSPIRE) / signature (INSPIRE) / magnetic field (INSPIRE) /
                      infrared (INSPIRE) / optical (INSPIRE) / GLAST (INSPIRE) /
                      accretion (INSPIRE)},
      cin          = {$Z_GA$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_GA-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613) /
                      MessMapp - Mapping Highly-Energetic Messengers throughout
                      the Universe (949555)},
      pid          = {G:(DE-HGF)POF4-613 / G:(EU-Grant)949555},
      experiment   = {EXP:(DE-H253)MAGIC-20170101},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)16},
      eprint       = {2403.13713},
      howpublished = {arXiv:2403.13713},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2403.13713;\%\%$},
      UT           = {WOS:001374323000001},
      doi          = {10.1093/mnras/stae2313},
      url          = {https://bib-pubdb1.desy.de/record/623126},
}