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The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes located on the canary island of La Palma. They provide the lowest energy threshold among existing instruments of the kind, reaching down to 50 GeV in standard trigger…

High Energy Astrophysical Phenomena · Physics 2022-03-02 S. Klepser

Aims. LST-1, the prototype of the Large-Sized Telescope for the upcoming Cherenkov Telescope Array Observatory, is concluding its commissioning in Observatorio del Roque de los Muchachos on the island of La Palma. The proximity of LST-1…

Instrumentation and Methods for Astrophysics · Physics 2023-12-13 H. Abe , K. Abe , S. Abe , V. A. Acciari , A. Aguasca-Cabot , I. Agudo , N. Alvarez Crespo , T. Aniello , S. Ansoldi , L. A. Antonelli , C. Aramo , A. Arbet-Engels , C. Arcaro , M. Artero , K. Asano , P. Aubert , D. Baack , A. Babić , A. Baktash , A. Bamba , A. Baquero Larriva , L. Baroncelli , U. Barres de Almeida , J. A. Barrio , I. Batković , J. Baxter , J. Becerra González , W. Bednarek , E. Bernardini , M. I. Bernardos , J. Bernete Medrano , A. Berti , J. Besenrieder , P. Bhattacharjee , N. Biederbeck , C. Bigongiari , A. Biland , E. Bissaldi , O. Blanch , G. Bonnoli , P. Bordas , Ž. Bošnjak , A. Bulgarelli , I. Burelli , L. Burmistrov , M. Buscemi , G. Busetto , A. Campoy Ordaz , M. Cardillo , S. Caroff , A. Carosi , R. Carosi , M. S. Carrasco , M. Carretero-Castrillo , F. Cassol , A. J. Castro-Tirado , D. Cauz , D. Cerasole , G. Ceribella , Y. Chai , K. Cheng , A. Chiavassa , M. Chikawa , L. Chytka , A. Cifuentes , S. Cikota , E. Colombo , J. L. Contreras , A. Cornelia , J. Cortina , H. Costantini , S. Covino , G. D'Amico , V. D'Elia , P. Da Vela , M. Dalchenko , F. Dazzi , A. De Angelis , M. de Bony de Lavergne , B. De Lotto , M. De Lucia , R. de Menezes , L. Del Peral , A. Del Popolo , G. Deleglise , M. Delfino , C. Delgado Mendez , J. Delgado Mengual , D. della Volpe , M. Dellaiera , D. Depaoli , A. De Angelis , A. Di Piano , F. Di Pierro , A. Di Pilato , R. Di Tria , L. Di Venere , R. M. Dominik , D. Dominis Prester , A. Donini , D. Dorner , M. Doro , C. Díaz , L. Eisenberger , D. Elsässer , G. Emery , J. Escudero , V. Fallah Ramazani , L. Fariña , A. Fattorini , G. Ferrara , F. Ferrarotto , A. Fiasson , L. Foffano , L. Font , L. Freixas Coromina , S. Fröse , S. Fukami , Y. Fukazawa , R. J. Garcia López , E. Garcia , M. Garczarczyk , R. J. García López , C. Gasbarra , D. Gasparrini , S. Gasparyan , M. Gaug , D. Geyer , J. G. Giesbrecht Paiva , N. Giglietto , F. Giordano , P. Gliwny , N. Godinović , R. Grau , D. Green , J. G. Green , S. Gunji , P. Günther , J. Hackfeld , D. Hadasch , A. Hahn , K. Hashiyama , T. Hassan , K. Hayashi , L. Heckmann , M. Heller , J. Herrera Llorente , K. Hirotani , D. Hoffmann , D. Horns , J. Houles , M. Hrabovsky , D. Hrupec , D. Hui , M. Hütten , M. Iarlori , R. Imazawa , T. Inada , Y. Inome , K. Ioka , M. Iori , R. Iotov , K. Ishio , M. Jacquemont , I. Jiménez Martínez , E. Jobst , J. Jormanainen , J. Jurysek , M. Kagaya , V. Karas , H. Katagiri , J. Kataoka , D. Kerszberg , G. W. Kluge , Y. Kobayashi , K. Kohri , A. Kong , P. M. Kouch , H. Kubo , J. Kushida , M. Lainez , G. Lamanna , A. Lamastra , T. Le Flour , F. Leone , E. Lindfors , L. Linhoff , M. Linhoff , S. Lombardi , F. Longo , S. Loporchio , A. Lorini , J. Lozano Bahilo , P. L. Luque-Escamilla , E. Lyard , M. Láinez Lezáun , R. López-Coto , M. López-Moya , A. López-Oramas , B. Machado de Oliveira Fraga , P. Majumdar , M. Makariev , D. Mandat , G. Maneva , M. Manganaro , S. Mangano , N. Mang , G. Manicò , K. Mannheim , M. Mariotti , P. Marquez , G. Marsella , O. Martinez , G. Martínez , M. Martínez , J. Martí , A. Mas-Aguilar , G. Maurin , D. Mazin , S. Menchiari , S. Mender , E. Mestre Guillen , S. Micanovic , D. Miceli , T. Miener , J. M. Miranda , R. Mirzoyan , T. Mizuno , S. Mićanović , M. Molero González , E. Molina , H. A. Mondal , T. Montaruli , I. Monteiro , A. Moralejo , D. Morcuende , A. Morselli , V. Moya , H. Muraishi , K. Murase , S. Nagataki , T. Nakamori , C. Nanci , A. Neronov , V. Neustroev , L. Nickel , M. Nievas Rosillo , C. Nigro , L. Nikolić , K. Nilsson , K. Nishijima , T. Njoh Ekoume , K. Noda , D. Nosek , S. Nozaki , M. Ohishi , Y. Ohtani , T. Oka , A. Okumura , R. Orito , J. Otero-Santos , S. Paiano , M. Palatiello , D. Paneque , F. R. Pantaleo , R. Paoletti , J. M. Paredes , L. Pavletić , M. Pech , M. Pecimotika , M. Peresano , M. Persic , F. Pfeiffle , E. Pietropaolo , M. Pihet , G. Pirola , C. Plard , F. Podobnik , V. Poireau , M. Polo , E. Pons , P. G. Prada Moroni , E. Prandini , J. Prast , G. Principe , C. Priyadarshi , M. Prouza , R. Rando , W. Rhode , M. Ribó , J. Rico , C. Righi , V. Rizi , G. Rodriguez Fernandez , M. D. Rodríguez Frías , N. Sahakyan , T. Saito , S. Sakurai , D. A. Sanchez , K. Satalecka , M. Sato , Y. Sato , F. G. Saturni , V. Savchenko , B. Schleicher , K. Schmidt , F. Schmuckermaier , J. L. Schubert , F. Schussler , T. Schweizer , A. Sciaccaluga , T. Siegert , R. Silvia , J. Sitarek , V. Sliusar , D. Sobczynska , A. Spolon , A. Stamerra , J. Strišković , D. Strom , M. Strzys , Y. Suda , S. Suutarinen , T. Šarić , H. Tajima , H. Takahashi , M. Takahashi , J. Takata , R. Takeishi , P. H. T. Tam , S. J. Tanaka , D. Tateishi , F. Tavecchio , P. Temnikov , Y. Terada , K. Terauchi , T. Terzić , M. Teshima , M. Tluczykont , F. Tokanai , D. F. Torres , L. Tosti , P. Travnicek , S. Truzzi , A. Tutone , S. Ubach , M. Vacula , P. Vallania , J. van Scherpenberg , M. Vazquez Acosta , S. Ventura , V. Verguilov , I. Viale , A. Vigliano , C. F. Vigorito , E. Visentin , V. Vitale , G. Voutsinas , I. Vovk , T. Vuillaume , M. Vázquez Acosta , R. Walter , Z. Wei , M. Will , T. Yamamoto , R. Yamazaki , T. Yoshida , T. Yoshikoshi , N. Zywucka

Current Imaging Atmospheric Cherenkov Telescopes for Very High Energy $\gamma$-ray astrophysics are pointing instruments with a Field of View up to a few tens of sq deg. We propose to build an array of two non-steerable (drift) telescopes.…

Instrumentation and Methods for Astrophysics · Physics 2015-08-26 J. Cortina , R. López-Coto , A. Moralejo

Imaging atmospheric Cherenkov telescopes (IACTs) are equipped with sensitive photomultiplier tube (PMT) cameras. Exposure to high levels of background illumination degrades the efficiency of and potentially destroys these photo-detectors…

The MAGIC 17m diameter Cherenkov telescope will be upgraded with a second telescope with advanced photon detectors and ultra fast readout within the year 2007. The sensitivity of MAGIC-II, the two telescope system, will be improved by a…

Astrophysics · Physics 2019-08-13 Florian Goebel

Context. We are operating an elastic LIDAR for the monitoring of atmospheric conditions during regular observations of the MAGIC Telescopes. Aims. We present and evaluate methods to convert aerosol extinction profiles, obtained with the…

With its diameter of 17m, the MAGIC telescope is the largest Cherenkov detector for gamma ray astrophysics. It is sensitive to photons above an energy of 30 GeV. MAGIC started operations in October 2003 and is currently taking data. This…

The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime…

Instrumentation and Methods for Astrophysics · Physics 2015-05-01 MAGIC Collaboration , J. Aleksic , S. Ansoldi , L. A. Antonelli , P. Antoranz , A. Babic , P. Bangale , M. Barcelo , J. A. Barrio , J. Becerra Gonzalez , W. Bednarek , E. Bernardini , B. Biasuzzi , A. Biland , M. Bitossi , O. Blanch , S. Bonnefoy , G. Bonnoli , F. Borracci , T. Bretz , E. Carmona , A. Carosi , R. Cecchi , P. Colin , E. Colombo , J. L. Contreras , D. Corti , J. Cortina , S. Covino , P. Da Vela , F. Dazzi , A. De Angelis , G. De Caneva , B. De Lotto , E. de Ona Wilhelmi , C. Delgado Mendez , A. Dettlaff , D. Dominis Prester , D. Dorner , M. Doro , S. Einecke , D. Eisenacher , D. Elsaesser , D. Fidalgo , D. Fink , M. V. Fonseca , L. Font , K. Frantzen , C. Fruck , D. Galindo , R. J. Garcia Lopez , M. Garczarczyk , D. Garrido Terrats , M. Gaug , G. Giavitto , N. Godinovic , A. Gonzalez Munoz , S. R. Gozzini , W. Haberer , D. Hadasch , Y. Hanabata , M. Hayashida , J. Herrera , D. Hildebrand , J. Hose , D. Hrupec , W. Idec , J. M. Illa , V. Kadenius , H. Kellermann , M. L. Knoetig , K. Kodani , Y. Konno , J. Krause , H. Kubo , J. Kushida , A. La Barbera , D. Lelas , J. L. Lemus , N. Lewandowska , E. Lindfors , S. Lombardi , F. Longo , M. Lopez , R. Lopez-Coto , A. Lopez-Oramas , A. Lorca , E. Lorenz , I. Lozano , M. Makariev , K. Mallot , G. Maneva , N. Mankuzhiyil , K. Mannheim , L. Maraschi , B. Marcote , M. Mariotti , M. Martinez , D. Mazin , U. Menzel , J. M. Miranda , R. Mirzoyan , A. Moralejo , P. Munar-Adrover , D. Nakajima , M. Negrello , V. Neustroev , A. Niedzwiecki , K. Nilsson , K. Nishijima , K. Noda , R. Orito , A. Overkemping , S. Paiano , M. Palatiello , D. Paneque , R. Paoletti , J. M. Paredes , X. Paredes-Fortuny , M. Persic , J. Poutanen , P. G. Prada Moroni , E. Prandini , I. Puljak , R. Reinthal , W. Rhode , M. Ribo , J. Rico , J. Rodriguez Garcia , S. Rugamer , T. Saito , K. Saito , K. Satalecka , V. Scalzotto , V. Scapin , C. Schultz , J. Schlammer , S. Schmidl , T. Schweizer , A. Sillanpaa , J. Sitarek , I. Snidaric , D. Sobczynska , F. Spanier , A. Stamerra , T. Steinbring , J. Storz , M. Strzys , L. Takalo , H. Takami , F. Tavecchio , L. A. Tejedor , P. Temnikov , T. Terzic , D. Tescaro , M. Teshima , J. Thaele , O. Tibolla , D. F. Torres , T. Toyama , A. Treves , P. Vogler , H. Wetteskind , M. Will , R. Zanin

MAGIC is a single-dish Cherenkov telescope located on La Palma (Spain), hence with an optimal view on the Northern sky. Sensitive in the 30 GeV-30 TeV energy band, it is nowadays the only ground-based instrument being able to measure…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Javier Rico , Robert Wagner

MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located on the Canary Island of La Palma and dedicated to the study of very high energy gamma rays above 30 GeV. MAGIC has recently demonstrated its capability as a neutrino…

High Energy Astrophysical Phenomena · Physics 2019-09-04 Manuela Mallamaci , Dariusz Gora , Elisa Bernardini

The paper describes the MAGIC multi-mode focal reducer (Monitoring of Active Galaxies by Investigation of their Cores), commissioned on the 1-m Zeiss-1000 telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences…

TeV Gamma-ray signals from the Crab Nebula and Mkn 501 were detected with the HEGRA CT1 imaging Cerenkov telescope during periods when the moon was shining and during twilight. This was accomplished by lowering the high voltage supply of…

Astrophysics · Physics 2009-10-31 D. Kranich , R. Mirzoyan , D. Petry , B. C. Raubenheimer

MAGIC is a system of two Cherenkov telescopes designed to perform observations of gamma rays with energies from about 50 GeV to tens of TeV. A low energy threshold and an excellent low energy performance make it a powerful instrument for…

High Energy Astrophysical Phenomena · Physics 2017-08-22 Julian Sitarek , the MAGIC Collaboration

We investigate the performance of the MAGIC telescopes under three simulated atmospheric conditions: an increased aerosol content in the lower part of the troposphere, the presence of thin aerosol over-densities at different heights, and an…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Daniel Garrido , Markus Gaug , Michele Doro , Lluís Font , Alicia López-Oramas , Abelardo Moralejo

The MAGIC telescope is the largest single-dish Imaging Atmospheric Cherenkov Telescope (IACT) with the lowest energy threshold among the current generation of IACTs as low as 25 GeV. Therefore, the MAGIC telescope is a perfect instrument to…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Roberta Zanin

The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) experiment is an array of two 17-meter telescopes located in the Canary Island of La Palma that observes the very-high energy (VHE) gamma-ray sky in stereoscopic mode since 2009.…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Ulisses Barres de Almeida

MAGIC, 17 meters of diameter, is the world's largest single dish Imaging Atmospheric Cherenkov Telescope, and reaches in the analysis the lowest energy threshold (60 GeV) among the VHE gamma detectors. Completed in September 2004, MAGIC…

Astrophysics · Physics 2007-08-28 MAGIC Collaboration , Alessandro De Angelis

MAGIC is a system of two 17-m diameter Imaging Atmospheric Cherenkov Telescopes, located at an altitude of 2200 m in Roque de los Muchachos on the Canary island of La Palma, exploring the gamma-ray sky above a few tens of GeV and up to tens…

High Energy Astrophysical Phenomena · Physics 2024-05-28 S. Mangano

In February 2007 the MAGIC Air Cherenkov Telescope for gamma-ray astronomy was fully upgraded with an ultra fast 2 GSamples/s digitization system. Since the Cherenkov light flashes are very short, a fast readout can minimize the influence…

A project to construct a 17 m diameter imaging air Cherenkov telescope, called the MAGIC Telescope, is described. The aim of the project is to close the observation gap in the gamma-ray sky extending from 10 GeV as the highest energy…

Astrophysics · Physics 2007-05-23 N. Magnussen