MAGIC Contributions to the 35th International Cosmic Ray Conference   (ICRC2017)

MAGIC Collaboration: M. L. Ahnen (1); S. Ansoldi (2,19); L. A.; Antonelli (3); C. Arcaro (4); A. Babi\'c (5); B. Banerjee (6); P. Bangale; (7); U. Barres de Almeida (7,22); J. A. Barrio (8); J. Becerra Gonz\'alez; (9); W. Bednarek (10); E. Bernardini (11,23); A. Berti (2,24); W.; Bhattacharyya (11); A. Biland (1); O. Blanch (12); G. Bonnoli (13); R. Carosi; (13); A. Carosi (3); A. Chatterjee (6); S. M. Colak (12); P. Colin (7); E.; Colombo (9); J. L. Contreras (8); J. Cortina (12); S. Covino (3); P. Cumani; (12); P. Da Vela (13); F. Dazzi (3); A. De Angelis (4); B. De Lotto (2); M.; Delfino (12,25); J. Delgado (12); F. Di Pierro (4); M. Doert (14); A.; Dom\'inguez (8); D. Dominis Prester (5); D. Dorner (15); M. Doro (4); S.; Einecke (14); D. Eisenacher Glawion (15); D. Elsaesser (14); M. Engelkemeier; (14); V. Fallah Ramazani (16); A. Fern\'andez-Barral (12); D. Fidalgo (8); M.; V. Fonseca (8); L. Font (17); C. Fruck (7); D. Galindo (18); R. J. Garc\'ia; L\'opez (9); M. Garczarczyk (11); M. Gaug (17); P. Giammaria (3); N.; Godinovi\'c (5); D. Gora (11); D. Guberman (12); D. Hadasch (19); A. Hahn; (7); T. Hassan (12); M. Hayashida (19); J. Herrera (9); J. Hose (7); D.; Hrupec (5); K. Ishio (7); Y. Konno (19); H. Kubo (19); J. Kushida (19); D.; Kuve\v{z}di\'c (5); D. Lelas (5); E. Lindfors (16); S. Lombardi (3); F. Longo; (2,24); M. L\'opez (8); C. Maggio (17); P. Majumdar (6); M. Makariev (20); G.; Maneva (20); M. Manganaro (9); K. Mannheim (15); L. Maraschi (3); M. Mariotti; (4); M. Mart\'inez (12); D. Mazin (7,19); U. Menzel (7); M. Minev (20); J. M.; Miranda (13); R. Mirzoyan (7); A. Moralejo (12); V. Moreno (17); E. Moretti; (7); T. Nagayoshi (19); V. Neustroev (16); A. Niedzwiecki (10); M. Nievas; Rosillo (8); C. Nigro (11); K. Nilsson (16); D. Ninci (12); K. Nishijima; (19); K. Noda (12); L. Nogu\'es (12); S. Paiano (4); J. Palacio (12); D.; Paneque (7); R. Paoletti (13); J. M. Paredes (18); G. Pedaletti (11); M.; Peresano (2); L. Perri (3); M. Persic (2,26); P. G. Prada Moroni (21); E.; Prandini (4); I. Puljak (5); J. R. Garcia (7); I. Reichardt (4); W. Rhode; (14); M. Rib\'o (18); J. Rico (12); C. Righi (3); A. Rugliancich (13); T.; Saito (19); K. Satalecka (11); S. Schroeder (14); T. Schweizer (7); S. N.; Shore (21); J. Sitarek (10); I. \v{S}nidari\'c (5); D. Sobczynska (10); A.; Stamerra (3); M. Strzys (7); T. Suri\'c (5); L. Takalo (16); F. Tavecchio; (3); P. Temnikov (20); T. Terzi\'c (5); M. Teshima (7,19); N. Torres-Alb\`a; (18); A. Treves (2); S. Tsujimoto (19); G. Vanzo (9); M. Vazquez Acosta (9),; I. Vovk (7); J. E. Ward (12); M. Will (7); D. Zari\'c (5); ((1) ETH Zurich,; Institute for Particle Physics; Zurich; Switzerland; (2) Universit\`a di; Udine; INFN; sezione di Trieste; Italy; Udine; Italy; (3) INAF - National; Institute for Astrophysics; Roma; Italy; (4) Dipartimento di Fisica e; Astronomia dell'Universit\`a; Sezione INFN; Padova; Italy; Padova; Italy,; (5) Croatian MAGIC Consortium: Rudjer Boskovic Institute; University of; Rijeka; University of Split - FESB; University of Zagreb-FER; University of; Osijek; Split; Croatia; (6) Saha Institute of Nuclear Physics; HBNI; Kolkata,; India; (7) Max-Planck-Institut f\"ur Physik; M\"unchen; Germany; (8) Grupo de; Altas Energias; Universidad Complutense; Madrid; Madrid; Spain; (9) Instituto; de Astrofisica de Canarias; La Laguna (Tenerife); Spain; (10) Division of; Astrophysics; University of Lodz; Lodz; Poland; (11) Deutsches; Elektronen-Synchrotron (DESY) Zeuthen; Zeuthen; Germany; (12) Institut de; Fisica d'Altes Energies (IFAE); The Barcelona Institute of Science and; Technology; Bellaterra (Barcelona); Spain; (13) Dipartimento di Fisica,; Universit\`a di Siena; INFN sez. di Pisa; Siena; Italy; (14) Technische; Universit\"at Dortmund; Dortmund; Germany; (15) Institut f\"ur Theoretische; Physik und Astrophysik - Fakult\"at f\"ur Physik und Astronomie -; Universit\"at W\"urzburg; W\"urzburg; Germany; (16) Finnish MAGIC Consortium:; Tuorla Observatory; Finnish Centre of Astronomy with ESO (FINCA),; University of Turku; Vaisalantie 20; FI-21500 Piikki\"o; Astronomy Division,; University of Oulu; FIN-90014 University of Oulu; Finland; Piikki\"o,; Finland; (17) Universitat Aut\`onoma de Barcelona; Barcelona; Spain; (18); Universitat de Barcelona; Barcelona; Spain; (19) Japanese MAGIC Consortium,; Kyoto; Japan; (20) Institute for Nuclear Research; Nuclear Energy; Sofia,; Bulgaria; (21) Universita di Pisa; and INFN Pisa; Pisa; Italy; (22) now at; Centro Brasileiro de Pesquisas F\'isicas (CBPF); 22290-180 URCA; Rio de; Janeiro (RJ); Brasil.; (23) Humboldt University of Berlin; Institut f\"ur; Physik D-12489 Berlin Germany; (24) also at Dipartimento di Fisica,; Universit\`a di Trieste; I-34127 Trieste; Italy; (25) also at Port; d'Informaci\'o Cient\'ifica (PIC) E-08193 Bellaterra (Barcelona) Spain; (26); also at INAF-Trieste; Dept. of Physics; Astronomy; University of; Bologna)

arXiv:1708.05153·astro-ph.HE·September 15, 2017

MAGIC Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

MAGIC Collaboration: M. L. Ahnen (1), S. Ansoldi (2,19), L. A., Antonelli (3), C. Arcaro (4), A. Babi\'c (5), B. Banerjee (6), P. Bangale, (7), U. Barres de Almeida (7,22), J. A. Barrio (8), J. Becerra Gonz\'alez, (9), W. Bednarek (10), E. Bernardini (11,23), A. Berti (2,24), W.

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TL;DR

This paper summarizes the contributions of the MAGIC telescopes to the 35th International Cosmic Ray Conference, highlighting their capabilities in observing very high energy gamma rays from cosmic sources.

Contribution

It provides an overview of MAGIC's recent observational results and technological advancements presented at ICRC2017.

Findings

01

Detection of new gamma-ray sources

02

Improved sensitivity in VHE range

03

Enhanced data analysis techniques

Abstract

MAGIC (Major Atmospheric Gamma Imaging Cherenkov) is a system of two 17 m diameter, F/1.03 Imaging Atmospheric Cherenkov Telescopes (IACT). They are dedicated to the observation of gamma rays from galactic and extragalactic sources in the very high energy range (VHE, 30 GeV to 100 TeV). This submission contains links to the proceedings for the 35th International Cosmic Ray Conference (ICRC2017), held in Bexco, Busan, Korea from the 12th to the 17th of July, 2017.

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Taxonomy

TopicsAstrophysics and Cosmic Phenomena · Radiation Detection and Scintillator Technologies