{"paper":{"title":"MAGIC detection of very high energy gamma-ray emission from the low-luminosity blazar 1ES 1741+196","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"(10) Inst. de Astrof\\'isica de Canarias, (11) University of \\L\\'od\\'z, (12) Deutsches Elektronen-Synchrotron (DESY), (13) Institut de Fisica d'Altes Energies (IFAE), (14) Universit\\\"at W\\\"urzburg, (15) Institute for Space Sciences (CSIC/IEEC), (16) Technische Universit\\\"at Dortmund, (17) Finnish MAGIC Consortium, (18) Unitat de F\\'isica de les Radiacions, (19) Universitat de Barcelona, 1/AF Bidhannagar, (20) Japanese MAGIC Consortium, (21) Inst. for Nucl. Research, (22) Universit\\`a di Pisa, (23) ICREA, 24), (24) also at the Department of Physics of Kyoto University, 25), (25) now at Centro Brasileiro de Pesquisas F\\'isicas (CBPF/MCTI), 26), (26) now at NASA Goddard Space Flight Center, 27), (27) Humboldt University of Berlin, 28), (28) also at University of Trieste, 29), (29) now at Ecole polytechnique f\\'ed\\'erale de Lausanne (EPFL), (2) Universit\\`a di Udine, 30), (30) now at Max-Planck-Institut fur Kernphysik, 31), (31) now at Astrophysical Sciences Division, 32), (32) also at Japanese MAGIC Consortium, 33), (33) now at Finnish Centre for Astronomy with ESO (FINCA), 34), (34) also at INAF-Trieste, 35), (35) also at ISDC - Science Data Center for Astrophysics, 36), (36) now at IPNS, (37) GRAPPA, 38), (38) ASI Science Data Center, (39) NASA Goddard Space Flight Center), (3) INAF National Institute for Astrophysics, (4) Universit\\`a di Siena, (5) Universit\\`a di Padova, (6) Croatian MAGIC Consortium, (7) Saha Institute of Nuclear Physics, (8) Max-Planck-Institut f\\\"ur Physik, (9) Universidad Complutense, A. Babic (6), A. Berti (2, A. Biland (1), A. Carosi (3), A. Chatterjee (7), A. De Angelis (5), A. Dom\\'inguez (9), A. Fern\\'andez-Barral (13), A. Hahn (8), A. La Barbera (3), A. Moralejo (13), A. Niedzwiecki (11), Anton Pannekoek Institute for Astronomy, A. Sillanp\\\"a\\\"a (17), A. Stamerra (3), Astronomy, Astronomy Division, A. Treves (2), BARC, B. Banerjee (7), B. Biasuzzi (2), B. De Lotto (2), B. Marcote (19), B. Rani (39), Campus UAB, C. Arcaro (5), CERES-IEEC, C. Fruck (8), Croatia, D. Dominis Prester (6), D. Dorner (14), D. Eisenacher Glawion (14), D. Elsaesser (16), Departament de F\\'isica, Department of Astronomy, Department of Physics, Dept. of Physics, D. Fidalgo (9), D. F. Torres (23), D. Galindo (19), D. Garrido Terrats (18), D. Gora (12), D. Guberman (13), D. Hadasch (20), D. Hrupec (6), D. Lelas (6), D. Mazin (8, D. Nakajima (20), D. Paneque (8), Dpto. Astrof\\'isica, D. Sobczynska (11), D. Tescaro (5), E. Bernardini (12, E. Colombo (10), E. de O\\~na Wilhelmi (15), E. Lindfors (17), E. Moretti (8), E. Prandini (1, F. Borracci (8), F. Dazzi (8), F. Di Pierro (3), Fermi-LAT collaboration: J. Becerra Gonz\\'alez (10, Finland, F. Krauss (37), F. Longo (2, F. Tavecchio (3), F. Verrecchia (3, G. Bonnoli (4), G. Hughes (1), G. Maneva (21), G. Pedaletti (12), Greenbelt, G. Vanzo (10), Hakubi Center, High Energy Accelerator Research Organization (KEK) 1-1 Oho, H. Kubo (20), H. Takami (20, ICC, ICRR, India, INFN, INFN Pisa, INFN Trieste, Institute for Space Sciences (CSIC/IEEC), Institut f\\\"ur Physik Newtonstr. 15, I. Puljak (6), I. Reichardt (5), I. Snidaric (6), I. Vovk (8), J. A. Barrio (9), Japan, J. Cortina (13), J. E. Ward (13), J. Herrera (10), J. Hose (8), J. Kushida (20), J. L. Contreras (9), J. M. Miranda (4), J. M. Paredes (19), J. Palacio (13), J. Poutanen (17), J. R. Garcia (8), J. Rico (13), J. Sitarek (11), K. Frantzen (16), K. Kodani (20), K. Mallot (12), K. Mannheim (14), K. Nilsson (17, K. Nishijima (20), K. Noda (8), K. Satalecka (12), Kyoto University, L. A. Antonelli (3), Lausanne, L. Font (18), L. Maraschi (3), L. Nogu\\'es (13), L. Perri (3), L. Takalo (17), MAGIC Collaboration: M. L. Ahnen (1), MD 20771, M. Doert (16), M. Doro (5), M. Engelkemeier (16), M. Garczarczyk (12), M. Gaug (18), M. Hayashida (20), M. H. Wu (15), M. L\\'opez (9), M. Makariev (21), M. Manganaro (10), M. Mariotti (5), M. Mart\\'inez (13), M. Nievas Rosillo (9), M. Palatiello (2), M. Peresano (2), M. Perri (3, M. Persic (2, M. Rib\\'o (19), M. Strzys (8), M. Teshima (8, Mumbai, M. V. Fonseca (9), M. Will (10), N. Godinovi\\'c (6), N. Mankuzhiyil (2, Nucl. Energy, O. Blanch (13), P. Antoranz (4), P. Bangale (8), P. Colin (8), P. Da Vela (4), P. Giammaria (3), P. G. Prada Moroni (22), P. Majumdar (7), P. Temnikov (21), R. Clavero (10), R. J. Garc\\'ia L\\'opez (10), R. L\\'opez-Coto (13, R. Mirzoyan (8), R. Paoletti (4), R. Reinthal (17) ((1) ETH Zurich, Rudjer Boskovic Institute, R. Zanin (19, S. Ansoldi (2, S. Bonnefoy (9), S. Buson (5, S. Covino (3), S. Einecke (16), S. Lombardi (3), S. N. Shore (22), S. Paiano (5), S. Schroeder (16), Switzerland, T. Bretz (14, Technology, The Barcelona Institute of Science, The University of Tokushima, The University of Tokyo, Tokai University, T. Saito (20), T. Schweizer (8), Tsukuba, T. Suri\\'c (6), T. Terzi\\'c (6), T. Toyama (8), Tuorla Observatory, Turku, U. Barres de Almeida (8, U. Menzel (8), Universidad de La Laguna, Universitat Aut\\`onoma de Barcelona, University of Amsterdam, University of Bologna, University of Maryland, University of Oulu, University of Rijeka, University of Split, University of Turku, University of Zagreb, USA, V. Fallah Ramazani (17), V. Neustroev (17), V. Verguilov (21), W. Bednarek (11), W. Idec (11), W. Rhode (16), X. Paredes-Fortuny (19), Y. Konno (20)","submitted_at":"2017-02-22T13:51:26Z","abstract_excerpt":"We present the first detection of the nearby (z=0.084) low-luminosity BL Lac object 1ES 1741+196 in the very high energy (VHE: E$>$100 GeV) band. This object lies in a triplet of interacting galaxies. Early predictions had suggested 1ES 1741+196 to be, along with several other high-frequency BL Lac sources, within the reach of MAGIC detectability. Its detection by MAGIC, later confirmed by VERITAS, helps to expand the small population of known TeV BL Lacs. The source was observed with the MAGIC telescopes between 2010 April and 2011 May, collecting 46 h of good quality data. These observations"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.06795","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}