J. Barranco Garcia - Max-Planck-Institut für Physik, D-80805 München, Germany

J. Barranco Garcia
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Name
J. Barranco Garcia
Affiliation
Max-Planck-Institut für Physik, D-80805 München, Germany
City
Munich
Country
Germany

Pubs By Year

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High Energy Astrophysical Phenomena (26)
 
Astrophysics of Galaxies (7)
 
Physics - Instrumentation and Detectors (5)
 
Instrumentation and Methods for Astrophysics (5)
 
High Energy Physics - Experiment (5)
 
Physics - Materials Science (4)
 
High Energy Physics - Theory (2)
 
Physics - Mesoscopic Systems and Quantum Hall Effect (2)
 
General Relativity and Quantum Cosmology (2)
 
Quantum Physics (2)
 
Cosmology and Nongalactic Astrophysics (2)
 
Physics - Optics (1)
 
Quantitative Biology - Neurons and Cognition (1)
 
Physics - Plasma Physics (1)
 
Mathematics - Information Theory (1)
 
Physics - Accelerator Physics (1)
 
Computer Science - Cryptography and Security (1)
 
Nonlinear Sciences - Chaotic Dynamics (1)
 
Physics - Classical Physics (1)
 
Computer Science - Distributed; Parallel; and Cluster Computing (1)
 
Computer Science - Networking and Internet Architecture (1)
 
Physics - Strongly Correlated Electrons (1)
 
Computer Science - Information Theory (1)

Publications Authored By J. Barranco Garcia

During 2003--2015, the CERN Axion Solar Telescope (CAST) has searched for $a\to\gamma$ conversion in the 9 T magnetic field of a refurbished LHC test magnet that can be directed toward the Sun. In its final phase of solar axion searches (2013--2015), CAST has returned to evacuated magnet pipes, which is optimal for small axion masses. The absence of a significant signal above background provides a world leading limit of $g_{a\gamma} < 0. Read More

The relativistic jets created by some active galactic nuclei are important agents of AGN feedback. In spite of this, our understanding of what produces these jets is still incomplete. X-ray observations, which can probe the processes operating in the central regions in immediate vicinity of the supermassive black hole, the presumed jet launching point, are potentially particularly valuable in illuminating the jet formation process. Read More

In this paper, He's frequency-amplitude formulation with some choice of location points that improve accuracy is applied to determine the periodic solution for the nonlinear oscillations of a punctual charge in the electric field of charged ring. The results of the present study are valid for small and large amplitudes of oscillation. The present method can be applied directly to highly nonlinear problems without any discretization, linearization or restrictive assumptions. Read More

2017Apr
Authors: MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, C. Arcaro4, A. Babić5, B. Banerjee6, P. Bangale7, U. Barres de Almeida8, J. A. Barrio9, J. Becerra González10, W. Bednarek11, E. Bernardini12, A. Berti13, W. Bhattacharyya14, B. Biasuzzi15, A. Biland16, O. Blanch17, S. Bonnefoy18, G. Bonnoli19, R. Carosi20, A. Carosi21, A. Chatterjee22, P. Colin23, E. Colombo24, J. L. Contreras25, J. Cortina26, S. Covino27, P. Cumani28, P. Da Vela29, F. Dazzi30, A. De Angelis31, B. De Lotto32, E. de Oña Wilhelmi33, F. Di Pierro34, M. Doert35, A. Domínguez36, D. Dominis Prester37, D. Dorner38, M. Doro39, S. Einecke40, D. Eisenacher Glawion41, D. Elsaesser42, M. Engelkemeier43, V. Fallah Ramazani44, A. Fernández-Barral45, D. Fidalgo46, M. V. Fonseca47, L. Font48, C. Fruck49, D. Galindo50, R. J. García López51, M. Garczarczyk52, M. Gaug53, P. Giammaria54, N. Godinović55, D. Gora56, S. Griffiths57, D. Guberman58, D. Hadasch59, A. Hahn60, T. Hassan61, M. Hayashida62, J. Herrera63, J. Hose64, D. Hrupec65, G. Hughes66, K. Ishio67, Y. Konno68, H. Kubo69, J. Kushida70, D. Kuveždić71, D. Lelas72, E. Lindfors73, S. Lombardi74, F. Longo75, M. López76, C. Maggio77, P. Majumdar78, M. Makariev79, G. Maneva80, M. Manganaro81, K. Mannheim82, L. Maraschi83, M. Mariotti84, M. Martínez85, D. Mazin86, U. Menzel87, M. Minev88, R. Mirzoyan89, A. Moralejo90, V. Moreno91, E. Moretti92, V. Neustroev93, A. Niedzwiecki94, M. Nievas Rosillo95, K. Nilsson96, D. Ninci97, K. Nishijima98, K. Noda99, L. Nogués100, S. Paiano101, J. Palacio102, D. Paneque103, R. Paoletti104, J. M. Paredes105, X. Paredes-Fortuny106, G. Pedaletti107, M. Peresano108, L. Perri109, M. Persic110, P. G. Prada Moroni111, E. Prandini112, I. Puljak113, J. R. Garcia114, I. Reichardt115, W. Rhode116, M. Ribó117, J. Rico118, T. Saito119, K. Satalecka120, S. Schroeder121, T. Schweizer122, S. N. Shore123, A. Sillanpää124, J. Sitarek125, I. Šnidarić126, D. Sobczynska127, A. Stamerra128, M. Strzys129, T. Surić130, L. Takalo131, F. Tavecchio132, P. Temnikov133, T. Terzić134, D. Tescaro135, M. Teshima136, D. F. Torres137, N. Torres-Albà138, A. Treves139, G. Vanzo140, M. Vazquez Acosta141, I. Vovk142, J. E. Ward143, M. Will144, D. Zarić145
Affiliations: 1ETH Zurich, Institute for Particle Physics, Zurich, Switzerland, 2Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 3INAF - National Institute for Astrophysics, Roma, Italy, 4Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 5Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 6Saha Institute of Nuclear Physics, HBNI, Kolkata, India, 7Max-Planck-Institut für Physik, München, Germany, 8Max-Planck-Institut für Physik, München, Germany, 9Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 10Instituto de Astrofisica de Canarias, La Laguna, 11Division of Astrophysics, University of Lodz, Lodz, Poland, 12Deutsches Elektronen-Synchrotron, 13Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 14Deutsches Elektronen-Synchrotron, 15Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 16ETH Zurich, Institute for Particle Physics, Zurich, Switzerland, 17Institut de Fisica d'Altes Energies, 18Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 19Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 20Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 21INAF - National Institute for Astrophysics, Roma, Italy, 22Saha Institute of Nuclear Physics, HBNI, Kolkata, India, 23Max-Planck-Institut für Physik, München, Germany, 24Instituto de Astrofisica de Canarias, La Laguna, 25Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 26Institut de Fisica d'Altes Energies, 27INAF - National Institute for Astrophysics, Roma, Italy, 28Institut de Fisica d'Altes Energies, 29Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 30INAF - National Institute for Astrophysics, Roma, Italy, 31Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 32Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 33Institut de Ciencies de l'Espai, 34Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 35Technische Universität Dortmund, Dortmund, Germany, 36Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 37Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 38Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 39Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 40Technische Universität Dortmund, Dortmund, Germany, 41Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 42Technische Universität Dortmund, Dortmund, Germany, 43Technische Universität Dortmund, Dortmund, Germany, 44Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 45Institut de Fisica d'Altes Energies, 46Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 47Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 48Universitat Autònoma de Barcelona, Barcelona, Spain, 49Max-Planck-Institut für Physik, München, Germany, 50Universitat de Barcelona, Barcelona, Spain, 51Instituto de Astrofisica de Canarias, La Laguna, 52Deutsches Elektronen-Synchrotron, 53Universitat Autònoma de Barcelona, Barcelona, Spain, 54INAF - National Institute for Astrophysics, Roma, Italy, 55Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 56Deutsches Elektronen-Synchrotron, 57Institut de Fisica d'Altes Energies, 58Institut de Fisica d'Altes Energies, 59Japanese MAGIC Consortium, Kyoto, Japan, 60Max-Planck-Institut für Physik, München, Germany, 61Institut de Fisica d'Altes Energies, 62Japanese MAGIC Consortium, Kyoto, Japan, 63Instituto de Astrofisica de Canarias, La Laguna, 64Max-Planck-Institut für Physik, München, Germany, 65Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 66ETH Zurich, Institute for Particle Physics, Zurich, Switzerland, 67Max-Planck-Institut für Physik, München, Germany, 68Japanese MAGIC Consortium, Kyoto, Japan, 69Japanese MAGIC Consortium, Kyoto, Japan, 70Japanese MAGIC Consortium, Kyoto, Japan, 71Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 72Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 73Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 74INAF - National Institute for Astrophysics, Roma, Italy, 75Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 76Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 77Universitat Autònoma de Barcelona, Barcelona, Spain, 78Saha Institute of Nuclear Physics, HBNI, Kolkata, India, 79Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, 80Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, 81Instituto de Astrofisica de Canarias, La Laguna, 82Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 83INAF - National Institute for Astrophysics, Roma, Italy, 84Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 85Institut de Fisica d'Altes Energies, 86Max-Planck-Institut für Physik, München, Germany, 87Max-Planck-Institut für Physik, München, Germany, 88Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, 89Max-Planck-Institut für Physik, München, Germany, 90Institut de Fisica d'Altes Energies, 91Universitat Autònoma de Barcelona, Barcelona, Spain, 92Max-Planck-Institut für Physik, München, Germany, 93Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 94Division of Astrophysics, University of Lodz, Lodz, Poland, 95Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 96Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 97Institut de Fisica d'Altes Energies, 98Japanese MAGIC Consortium, Kyoto, Japan, 99Institut de Fisica d'Altes Energies, 100Institut de Fisica d'Altes Energies, 101Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 102Institut de Fisica d'Altes Energies, 103Max-Planck-Institut für Physik, München, Germany, 104Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 105Universitat de Barcelona, Barcelona, Spain, 106Universitat de Barcelona, Barcelona, Spain, 107Deutsches Elektronen-Synchrotron, 108Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 109INAF - National Institute for Astrophysics, Roma, Italy, 110Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 111Universita di Pisa, and INFN Pisa, Pisa, Italy, 112Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 113Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 114Max-Planck-Institut für Physik, München, Germany, 115Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 116Technische Universität Dortmund, Dortmund, Germany, 117Universitat de Barcelona, Barcelona, Spain, 118Institut de Fisica d'Altes Energies, 119Japanese MAGIC Consortium, Kyoto, Japan, 120Deutsches Elektronen-Synchrotron, 121Technische Universität Dortmund, Dortmund, Germany, 122Max-Planck-Institut für Physik, München, Germany, 123Universita di Pisa, and INFN Pisa, Pisa, Italy, 124Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 125Division of Astrophysics, University of Lodz, Lodz, Poland, 126Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 127Division of Astrophysics, University of Lodz, Lodz, Poland, 128INAF - National Institute for Astrophysics, Roma, Italy, 129Max-Planck-Institut für Physik, München, Germany, 130Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 131Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 132INAF - National Institute for Astrophysics, Roma, Italy, 133Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, 134Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 135Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 136Max-Planck-Institut für Physik, München, Germany, 137ICREA and Institut de Ciencies de l'Espai, 138Universitat de Barcelona, Barcelona, Spain, 139Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 140Instituto de Astrofisica de Canarias, La Laguna, 141Instituto de Astrofisica de Canarias, La Laguna, 142Max-Planck-Institut für Physik, München, Germany, 143Institut de Fisica d'Altes Energies, 144Instituto de Astrofisica de Canarias, La Laguna, 145Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia

MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Read More

We disentangle X-ray disk reflection from complex line-of-sight absorption in the nearby Seyfert NGC 4151, using a suite of Suzaku, NuSTAR, and XMM-Newton observations. Extending upon earlier published work, we pursue a physically motivated model using the latest angle-resolved version of the lamp-post geometry reflection model relxillCp_lp together with a Comptonization continuum. We use the long-look simultaneous Suzaku/NuSTAR observation to develop a baseline model wherein we model reflected emission as a combination of lamp-post components at the heights of 1. Read More

Ark 564 is an archetypal Narrow line Seyfert 1 that has been well observed in soft X-rays from 0.3-10 keV, revealing a steep spectrum, strong soft excess, iron K emission line and dramatic variability on the order of hours. Because of its very steep spectrum, observations of the source above 10 keV have been sparse. Read More

2017Mar
Authors: M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, C. Arcaro4, A. Babić5, B. Banerjee6, P. Bangale7, U. Barres de Almeida8, J. A. Barrio9, J. Becerra González10, W. Bednarek11, E. Bernardini12, A. Berti13, B. Biasuzzi14, A. Biland15, O. Blanch16, S. Bonnefoy17, G. Bonnoli18, F. Borracci19, T. Bretz20, R. Carosi21, A. Carosi22, A. Chatterjee23, P. Colin24, E. Colombo25, J. L. Contreras26, J. Cortina27, S. Covino28, P. Cumani29, P. Da Vela30, F. Dazzi31, A. De Angelis32, B. De Lotto33, E. de Oña Wilhelmi34, F. Di Pierro35, M. Doert36, A. Domínguez37, D. Dominis Prester38, D. Dorner39, M. Doro40, S. Einecke41, D. Eisenacher Glawion42, D. Elsaesser43, M. Engelkemeier44, V. Fallah Ramazani45, A. Fernández-Barral46, D. Fidalgo47, M. V. Fonseca48, L. Font49, C. Fruck50, D. Galindo51, R. J. García López52, M. Garczarczyk53, M. Gaug54, P. Giammaria55, N. Godinović56, D. Gora57, D. Guberman58, D. Hadasch59, A. Hahn60, T. Hassan61, M. Hayashida62, J. Herrera63, J. Hose64, D. Hrupec65, G. Hughes66, W. Idec67, K. Ishio68, K. Kodani69, Y. Konno70, H. Kubo71, J. Kushida72, D. Lelas73, E. Lindfors74, S. Lombardi75, F. Longo76, M. López77, P. Majumdar78, M. Makariev79, K. Mallot80, G. Maneva81, M. Manganaro82, K. Mannheim83, L. Maraschi84, M. Mariotti85, M. Martínez86, D. Mazin87, U. Menzel88, R. Mirzoyan89, A. Moralejo90, E. Moretti91, D. Nakajima92, V. Neustroev93, A. Niedzwiecki94, M. Nievas Rosillo95, K. Nilsson96, K. Nishijima97, K. Noda98, L. Nogués99, M. Nöthe100, S. Paiano101, J. Palacio102, D. Paneque103, R. Paoletti104, J. M. Paredes105, X. Paredes-Fortuny106, G. Pedaletti107, M. Peresano108, L. Perri109, M. Persic110, J. Poutanen111, P. G. Prada Moroni112, E. Prandini113, I. Puljak114, J. R. Garcia115, I. Reichardt116, W. Rhode117, M. Ribó118, J. Rico119, T. Saito120, K. Satalecka121, S. Schroeder122, T. Schweizer123, S. N. Shore124, A. Sillanpää125, J. Sitarek126, I. Šnidarić127, D. Sobczynska128, A. Stamerra129, M. Strzys130, T. Surić131, L. Takalo132, F. Tavecchio133, P. Temnikov134, T. Terzić135, D. Tescaro136, M. Teshima137, D. F. Torres138, N. Torres-Albà139, T. Toyama140, A. Treves141, G. Vanzo142, M. Vazquez Acosta143, I. Vovk144, J. E. Ward145, M. Will146, M. H. Wu147, F. Krauß148, R. Schulz149, M. Kadler150, J. Wilms151, E. Ros152, U. Bach153, T. Beuchert154, M. Langejahn155, C. Wendel156, N. Gehrels157, W. H. Baumgartner158, C. B. Markwardt159, C. Müller160, V. Grinberg161, T. Hovatta162, J. Magill163
Affiliations: 1ETH Zurich, Institute for Particle Physics, Zurich, Switzerland, 2Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 3INAF - National Institute for Astrophysics, Roma, Italy, 4Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 5Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 6Saha Institute of Nuclear Physics, HBNI, Kolkata, India, 7Max-Planck-Institut für Physik, München, Germany, 8Max-Planck-Institut für Physik, München, Germany, 9Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 10Instituto de Astrofisica de Canarias, La Laguna, 11Division of Astrophysics, University of Lodz, Lodz, Poland, 12Deutsches Elektronen-Synchrotron, 13Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 14Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 15ETH Zurich, Institute for Particle Physics, Zurich, Switzerland, 16Institut de Fisica d'Altes Energies, 17Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 18Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 19Max-Planck-Institut für Physik, München, Germany, 20Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 21Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 22INAF - National Institute for Astrophysics, Roma, Italy, 23Saha Institute of Nuclear Physics, HBNI, Kolkata, India, 24Max-Planck-Institut für Physik, München, Germany, 25Instituto de Astrofisica de Canarias, La Laguna, 26Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 27Institut de Fisica d'Altes Energies, 28INAF - National Institute for Astrophysics, Roma, Italy, 29Institut de Fisica d'Altes Energies, 30Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 31Max-Planck-Institut für Physik, München, Germany, 32Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 33Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 34Institut de Ciencies de l'Espai, 35INAF - National Institute for Astrophysics, Roma, Italy, 36Technische Universität Dortmund, Dortmund, Germany, 37Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 38Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 39Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 40Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 41Technische Universität Dortmund, Dortmund, Germany, 42Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 43Technische Universität Dortmund, Dortmund, Germany, 44Technische Universität Dortmund, Dortmund, Germany, 45Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 46Institut de Fisica d'Altes Energies, 47Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 48Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 49Universitat Autònoma de Barcelona, Barcelona, Spain, 50Max-Planck-Institut für Physik, München, Germany, 51Universitat de Barcelona, Barcelona, Spain, 52Instituto de Astrofisica de Canarias, La Laguna, 53Deutsches Elektronen-Synchrotron, 54Universitat Autònoma de Barcelona, Barcelona, Spain, 55INAF - National Institute for Astrophysics, Roma, Italy, 56Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 57Deutsches Elektronen-Synchrotron, 58Institut de Fisica d'Altes Energies, 59Japanese MAGIC Consortium, Kyoto, Japan, 60Max-Planck-Institut für Physik, München, Germany, 61Institut de Fisica d'Altes Energies, 62Japanese MAGIC Consortium, Kyoto, Japan, 63Instituto de Astrofisica de Canarias, La Laguna, 64Max-Planck-Institut für Physik, München, Germany, 65Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 66ETH Zurich, Institute for Particle Physics, Zurich, Switzerland, 67Division of Astrophysics, University of Lodz, Lodz, Poland, 68Max-Planck-Institut für Physik, München, Germany, 69Japanese MAGIC Consortium, Kyoto, Japan, 70Japanese MAGIC Consortium, Kyoto, Japan, 71Japanese MAGIC Consortium, Kyoto, Japan, 72Japanese MAGIC Consortium, Kyoto, Japan, 73Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 74Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 75INAF - National Institute for Astrophysics, Roma, Italy, 76Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 77Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 78Saha Institute of Nuclear Physics, HBNI, Kolkata, India, 79Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, 80Deutsches Elektronen-Synchrotron, 81Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, 82Instituto de Astrofisica de Canarias, La Laguna, 83Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 84INAF - National Institute for Astrophysics, Roma, Italy, 85Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 86Institut de Fisica d'Altes Energies, 87Max-Planck-Institut für Physik, München, Germany, 88Max-Planck-Institut für Physik, München, Germany, 89Max-Planck-Institut für Physik, München, Germany, 90Institut de Fisica d'Altes Energies, 91Max-Planck-Institut für Physik, München, Germany, 92Japanese MAGIC Consortium, Kyoto, Japan, 93Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 94Division of Astrophysics, University of Lodz, Lodz, Poland, 95Grupo de Altas Energias, Universidad Complutense, Madrid, Madrid, Spain, 96Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 97Japanese MAGIC Consortium, Kyoto, Japan, 98Max-Planck-Institut für Physik, München, Germany, 99Institut de Fisica d'Altes Energies, 100Technische Universität Dortmund, Dortmund, Germany, 101Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 102Institut de Fisica d'Altes Energies, 103Max-Planck-Institut für Physik, München, Germany, 104Dipartimento di Fisica, Università di Siena and INFN sez. di Pisa, Siena, Italy, 105Universitat de Barcelona, Barcelona, Spain, 106Universitat de Barcelona, Barcelona, Spain, 107Deutsches Elektronen-Synchrotron, 108Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 109INAF - National Institute for Astrophysics, Roma, Italy, 110Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 111Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 112Universita di Pisa, and INFN Pisa, Pisa, Italy, 113Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 114Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 115Max-Planck-Institut für Physik, München, Germany, 116Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 117Technische Universität Dortmund, Dortmund, Germany, 118Universitat de Barcelona, Barcelona, Spain, 119Institut de Fisica d'Altes Energies, 120Japanese MAGIC Consortium, Kyoto, Japan, 121Deutsches Elektronen-Synchrotron, 122Technische Universität Dortmund, Dortmund, Germany, 123Max-Planck-Institut für Physik, München, Germany, 124Universita di Pisa, and INFN Pisa, Pisa, Italy, 125Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 126Division of Astrophysics, University of Lodz, Lodz, Poland, 127Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 128Division of Astrophysics, University of Lodz, Lodz, Poland, 129INAF - National Institute for Astrophysics, Roma, Italy, 130Max-Planck-Institut für Physik, München, Germany, 131Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 132Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, Piikkiö, Finland, 133INAF - National Institute for Astrophysics, Roma, Italy, 134Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria, 135Croatian MAGIC Consortium: Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb-FER, University of Osijek, Split, Croatia, 136Dipartimento di Fisica ed Astronomia, Università di Padova and INFN sez. di Padova, Padova, Italy, 137Max-Planck-Institut für Physik, München, Germany, 138ICREA and Institut de Ciencies de l'Espai, 139Universitat de Barcelona, Barcelona, Spain, 140Max-Planck-Institut für Physik, München, Germany, 141Università di Udine and INFN, sezione di Trieste, Italy, Udine, Italy, 142Instituto de Astrofisica de Canarias, La Laguna, 143Instituto de Astrofisica de Canarias, La Laguna, 144Max-Planck-Institut für Physik, München, Germany, 145Institut de Fisica d'Altes Energies, 146Instituto de Astrofisica de Canarias, La Laguna, 147Institut de Ciencies de l'Espai, 148GRAPPA and Anton Pannekoek Institute for Astronomy, University of Amsterdam, The Netherlands, 149ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, 150Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 151Dr. Remeis Sternwarte and ECAP, Universität Erlangen-Nürnberg, Bamberg, Germany, 152Max-Planck-Institut für Radioastronomie, Bonn, Germany, 153Max-Planck-Institut für Radioastronomie, Bonn, Germany, 154Dr. Remeis Sternwarte and ECAP, Universität Erlangen-Nürnberg, Bamberg, Germany, 155Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 156Institut für Theoretische Physik und Astrophysik - Fakultät für Physik und Astronomie - Universität Würzburg, Würzburg, Germany, 157NASA, Goddard Space Flight Center, Greenbelt, USA, 158NASA, Goddard Space Flight Center, Greenbelt, USA, 159NASA, Goddard Space Flight Center, Greenbelt, USA, 160Department of Astrophysics/IMAPP, Radboud University Nijmegen, Nijmegen, the Netherlands, 161Massachusetts Institute of Technology, Kavli Institute for Astrophysics and Space Research, Cambridge, USA, 162Aalto University Metsähovi Radio Observatory, Kylmälä, Finland, 163Department of Physics and Department of Astronomy, University of Maryland, College Park, USA)

The extragalactic VHE gamma-ray sky is rich in blazars. These are jetted active galactic nuclei viewed at a small angle to the line-of-sight. Only a handful of objects viewed at a larger angle are known so far to emit above 100 GeV. Read More

Many of the services a smart city can provide to its citizens rely on the ability of its infrastructure to collect and process in real time vast amounts of continuous data that sensors deployed through the city produce. In this paper we present the server infrastructure we have designed in the context of the HERMES project to collect the data from sensors and aggregate it in streams for their use in services of the smart city. Read More

Active galactic nucleus (AGN) feedback is the process by which supermassive black holes in the centres of galaxies may moderate the growth of their hosts. Gas outflows from supermassive black holes release huge quantities of energy into the interstellar medium, clearing the surrounding gas. The most extreme of these, the ultra-fast outflows (UFOs), are the subset of X-ray detected outflows with velocities higher than 10,000 km/s, believed to originate in relativistic disc winds, a few hundred gravitational radii from the black hole. Read More

2017Feb
Authors: MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, P. Antoranz4, C. Arcaro5, A. Babic6, B. Banerjee7, P. Bangale8, U. Barres de Almeida9, J. A. Barrio10, J. Becerra González11, W. Bednarek12, E. Bernardini13, A. Berti14, B. Biasuzzi15, A. Biland16, O. Blanch17, S. Bonnefoy18, G. Bonnoli19, F. Borracci20, T. Bretz21, R. Carosi22, A. Carosi23, A. Chatterjee24, P. Colin25, E. Colombo26, J. L. Contreras27, J. Cortina28, S. Covino29, P. Cumani30, P. Da Vela31, F. Dazzi32, A. De Angelis33, B. De Lotto34, E. de Oña Wilhelmi35, F. Di Pierro36, M. Doert37, A. Domínguez38, D. Dominis Prester39, D. Dorner40, M. Doro41, S. Einecke42, D. Eisenacher Glawion43, D. Elsaesser44, M. Engelkemeier45, V. Fallah Ramazani46, A. Fernández-Barral47, D. Fidalgo48, M. V. Fonseca49, L. Font50, K. Frantzen51, C. Fruck52, D. Galindo53, R. J. García López54, M. Garczarczyk55, D. Garrido Terrats56, M. Gaug57, P. Giammaria58, N. Godinović59, D. Gora60, D. Guberman61, D. Hadasch62, A. Hahn63, M. Hayashida64, J. Herrera65, J. Hose66, D. Hrupec67, G. Hughes68, W. Idec69, K. Kodani70, Y. Konno71, H. Kubo72, J. Kushida73, A. La Barbera74, D. Lelas75, E. Lindfors76, S. Lombardi77, F. Longo78, M. López79, R. López-Coto80, P. Majumdar81, M. Makariev82, K. Mallot83, G. Maneva84, M. Manganaro85, K. Mannheim86, L. Maraschi87, B. Marcote88, M. Mariotti89, M. Martínez90, D. Mazin91, U. Menzel92, J. M. Miranda93, R. Mirzoyan94, A. Moralejo95, E. Moretti96, D. Nakajima97, V. Neustroev98, A. Niedzwiecki99, M. Nievas Rosillo100, K. Nilsson101, K. Nishijima102, K. Noda103, L. Nogués104, S. Paiano105, J. Palacio106, M. Palatiello107, D. Paneque108, R. Paoletti109, J. M. Paredes110, X. Paredes-Fortuny111, G. Pedaletti112, M. Peresano113, L. Perri114, M. Persic115, J. Poutanen116, P. G. Prada Moroni117, E. Prandini118, I. Puljak119, J. R. Garcia120, I. Reichardt121, W. Rhode122, M. Ribó123, J. Rico124, T. Saito125, K. Satalecka126, S. Schroeder127, T. Schweizer128, A. Sillanpää129, J. Sitarek130, I. Snidaric131, D. Sobczynska132, A. Stamerra133, M. Strzys134, T. Surić135, L. Takalo136, F. Tavecchio137, P. Temnikov138, T. Terzić139, D. Tescaro140, M. Teshima141, D. F. Torres142, T. Toyama143, A. Treves144, G. Vanzo145, M. Vazquez Acosta146, I. Vovk147, J. E. Ward148, M. Will149, M. H. Wu150, R. Zanin151
Affiliations: 1ETH Zurich, CH-8093 Zurich, Switzerland, 2Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 3INAF National Institute for Astrophysics, I-00136 Rome, Italy, 4Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 5Università di Padova and INFN, I-35131 Padova, Italy, 6Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 7Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 8Max-Planck-Institut für Physik, D-80805 München, Germany, 9Max-Planck-Institut für Physik, D-80805 München, Germany, 10Universidad Complutense, E-28040 Madrid, Spain, 11Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 12University of Łódź, PL-90236 Lodz, Poland, 13Deutsches Elektronen-Synchrotron, 14Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 15Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 16ETH Zurich, CH-8093 Zurich, Switzerland, 17Institut de Fisica d'Altes Energies, 18Universidad Complutense, E-28040 Madrid, Spain, 19Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 20Max-Planck-Institut für Physik, D-80805 München, Germany, 21Universität Würzburg, D-97074 Würzburg, Germany, 22Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 23INAF National Institute for Astrophysics, I-00136 Rome, Italy, 24Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 25Max-Planck-Institut für Physik, D-80805 München, Germany, 26Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 27Universidad Complutense, E-28040 Madrid, Spain, 28Institut de Fisica d'Altes Energies, 29INAF National Institute for Astrophysics, I-00136 Rome, Italy, 30Institut de Fisica d'Altes Energies, 31Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 32Max-Planck-Institut für Physik, D-80805 München, Germany, 33Università di Padova and INFN, I-35131 Padova, Italy, 34Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 35Institute for Space Sciences, 36INAF National Institute for Astrophysics, I-00136 Rome, Italy, 37Technische Universität Dortmund, D-44221 Dortmund, Germany, 38Universidad Complutense, E-28040 Madrid, Spain, 39Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 40Universität Würzburg, D-97074 Würzburg, Germany, 41Università di Padova and INFN, I-35131 Padova, Italy, 42Technische Universität Dortmund, D-44221 Dortmund, Germany, 43Universität Würzburg, D-97074 Würzburg, Germany, 44Technische Universität Dortmund, D-44221 Dortmund, Germany, 45Technische Universität Dortmund, D-44221 Dortmund, Germany, 46Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 47Institut de Fisica d'Altes Energies, 48Universidad Complutense, E-28040 Madrid, Spain, 49Universidad Complutense, E-28040 Madrid, Spain, 50Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 51Technische Universität Dortmund, D-44221 Dortmund, Germany, 52Max-Planck-Institut für Physik, D-80805 München, Germany, 53Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 54Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 55Deutsches Elektronen-Synchrotron, 56Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 57Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 58INAF National Institute for Astrophysics, I-00136 Rome, Italy, 59Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 60Deutsches Elektronen-Synchrotron, 61Institut de Fisica d'Altes Energies, 62Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 63Max-Planck-Institut für Physik, D-80805 München, Germany, 64Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 65Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 66Max-Planck-Institut für Physik, D-80805 München, Germany, 67Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 68ETH Zurich, CH-8093 Zurich, Switzerland, 69University of Łódź, PL-90236 Lodz, Poland, 70Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 71Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 72Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 73Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 74INAF National Institute for Astrophysics, I-00136 Rome, Italy, 75Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 76Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 77INAF National Institute for Astrophysics, I-00136 Rome, Italy, 78Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 79Universidad Complutense, E-28040 Madrid, Spain, 80Institut de Fisica d'Altes Energies, 81Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 82Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 83Deutsches Elektronen-Synchrotron, 84Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 85Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 86Universität Würzburg, D-97074 Würzburg, Germany, 87INAF National Institute for Astrophysics, I-00136 Rome, Italy, 88Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 89Università di Padova and INFN, I-35131 Padova, Italy, 90Institut de Fisica d'Altes Energies, 91Max-Planck-Institut für Physik, D-80805 München, Germany, 92Max-Planck-Institut für Physik, D-80805 München, Germany, 93Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 94Max-Planck-Institut für Physik, D-80805 München, Germany, 95Institut de Fisica d'Altes Energies, 96Max-Planck-Institut für Physik, D-80805 München, Germany, 97Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 98Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 99University of Łódź, PL-90236 Lodz, Poland, 100Universidad Complutense, E-28040 Madrid, Spain, 101Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 102Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 103Max-Planck-Institut für Physik, D-80805 München, Germany, 104Institut de Fisica d'Altes Energies, 105Università di Padova and INFN, I-35131 Padova, Italy, 106Institut de Fisica d'Altes Energies, 107Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 108Max-Planck-Institut für Physik, D-80805 München, Germany, 109Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 110Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 111Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 112Deutsches Elektronen-Synchrotron, 113Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 114INAF National Institute for Astrophysics, I-00136 Rome, Italy, 115Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 116Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 117Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy, 118ETH Zurich, CH-8093 Zurich, Switzerland, 119Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 120Max-Planck-Institut für Physik, D-80805 München, Germany, 121Università di Padova and INFN, I-35131 Padova, Italy, 122Technische Universität Dortmund, D-44221 Dortmund, Germany, 123Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 124Institut de Fisica d'Altes Energies, 125Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 126Deutsches Elektronen-Synchrotron, 127Technische Universität Dortmund, D-44221 Dortmund, Germany, 128Max-Planck-Institut für Physik, D-80805 München, Germany, 129Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 130University of Łódź, PL-90236 Lodz, Poland, 131Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 132University of Łódź, PL-90236 Lodz, Poland, 133INAF National Institute for Astrophysics, I-00136 Rome, Italy, 134Max-Planck-Institut für Physik, D-80805 München, Germany, 135Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 136Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 137INAF National Institute for Astrophysics, I-00136 Rome, Italy, 138Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 139Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 140Università di Padova and INFN, I-35131 Padova, Italy, 141Max-Planck-Institut für Physik, D-80805 München, Germany, 142ICREA and Institute for Space Sciences, 143Max-Planck-Institut für Physik, D-80805 München, Germany, 144Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 145Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 146Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 147Max-Planck-Institut für Physik, D-80805 München, Germany, 148Institut de Fisica d'Altes Energies, 149Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, 150Institute for Space Sciences, 151Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain

In this work we present data from observations with the MAGIC telescopes of SN 2014J detected in January 21 2014, the closest Type Ia supernova since Imaging Air Cherenkov Telescopes started to operate. We probe the possibility of very-high-energy (VHE; $E\geq100$ GeV) gamma rays produced in the early stages of Type Ia supernova explosions. We performed follow-up observations after this supernova explosion for 5 days, between January 27 and February 2 in 2014. Read More

2017Feb
Authors: MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, P. Antoranz4, C. Arcaro5, A. Babic6, B. Banerjee7, P. Bangale8, U. Barres de Almeida9, J. A. Barrio10, W. Bednarek11, E. Bernardini12, A. Berti13, B. Biasuzzi14, A. Biland15, O. Blanch16, S. Bonnefoy17, G. Bonnoli18, F. Borracci19, T. Bretz20, S. Buson21, A. Carosi22, A. Chatterjee23, R. Clavero24, P. Colin25, E. Colombo26, J. L. Contreras27, J. Cortina28, S. Covino29, P. Da Vela30, F. Dazzi31, A. De Angelis32, B. De Lotto33, E. de Oña Wilhelmi34, F. Di Pierro35, M. Doert36, A. Domínguez37, D. Dominis Prester38, D. Dorner39, M. Doro40, S. Einecke41, D. Eisenacher Glawion42, D. Elsaesser43, M. Engelkemeier44, V. Fallah Ramazani45, A. Fernández-Barral46, D. Fidalgo47, M. V. Fonseca48, L. Font49, K. Frantzen50, C. Fruck51, D. Galindo52, R. J. García López53, M. Garczarczyk54, D. Garrido Terrats55, M. Gaug56, P. Giammaria57, N. Godinović58, D. Gora59, D. Guberman60, D. Hadasch61, A. Hahn62, M. Hayashida63, J. Herrera64, J. Hose65, D. Hrupec66, G. Hughes67, W. Idec68, K. Kodani69, Y. Konno70, H. Kubo71, J. Kushida72, A. La Barbera73, D. Lelas74, E. Lindfors75, S. Lombardi76, F. Longo77, M. López78, R. López-Coto79, P. Majumdar80, M. Makariev81, K. Mallot82, G. Maneva83, M. Manganaro84, N. Mankuzhiyil85, K. Mannheim86, L. Maraschi87, B. Marcote88, M. Mariotti89, M. Martínez90, D. Mazin91, U. Menzel92, J. M. Miranda93, R. Mirzoyan94, A. Moralejo95, E. Moretti96, D. Nakajima97, V. Neustroev98, A. Niedzwiecki99, M. Nievas Rosillo100, K. Nilsson101, K. Nishijima102, K. Noda103, L. Nogués104, S. Paiano105, J. Palacio106, M. Palatiello107, D. Paneque108, R. Paoletti109, J. M. Paredes110, X. Paredes-Fortuny111, G. Pedaletti112, M. Peresano113, L. Perri114, M. Persic115, J. Poutanen116, P. G. Prada Moroni117, E. Prandini118, I. Puljak119, J. R. Garcia120, I. Reichardt121, W. Rhode122, M. Ribó123, J. Rico124, T. Saito125, K. Satalecka126, S. Schroeder127, T. Schweizer128, S. N. Shore129, A. Sillanpää130, J. Sitarek131, I. Snidaric132, D. Sobczynska133, A. Stamerra134, M. Strzys135, T. Surić136, L. Takalo137, H. Takami138, F. Tavecchio139, P. Temnikov140, T. Terzić141, D. Tescaro142, M. Teshima143, D. F. Torres144, T. Toyama145, A. Treves146, G. Vanzo147, V. Verguilov148, I. Vovk149, J. E. Ward150, M. Will151, M. H. Wu152, R. Zanin153, Fermi-LAT collaboration154, :155, J. Becerra González156, B. Rani157, F. Krauss158, M. Perri159, F. Verrecchia160, R. Reinthal161
Affiliations: 1ETH Zurich, 2Università di Udine, INFN Trieste, 3INAF National Institute for Astrophysics, 4Università di Siena, INFN Pisa, 5Università di Padova and INFN, 6Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 7Saha Institute of Nuclear Physics, 1/AF Bidhannagar, 8Max-Planck-Institut für Physik, 9Max-Planck-Institut für Physik, 10Universidad Complutense, 11University of Łódź, 12Deutsches Elektronen-Synchrotron, 13Università di Udine, INFN Trieste, 14Università di Udine, INFN Trieste, 15ETH Zurich, 16Institut de Fisica d'Altes Energies, 17Universidad Complutense, 18Università di Siena, INFN Pisa, 19Max-Planck-Institut für Physik, 20Universität Würzburg, 21Università di Padova and INFN, 22INAF National Institute for Astrophysics, 23Saha Institute of Nuclear Physics, 1/AF Bidhannagar, 24Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 25Max-Planck-Institut für Physik, 26Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 27Universidad Complutense, 28Institut de Fisica d'Altes Energies, 29INAF National Institute for Astrophysics, 30Università di Siena, INFN Pisa, 31Max-Planck-Institut für Physik, 32Università di Padova and INFN, 33Università di Udine, INFN Trieste, 34Institute for Space Sciences, 35INAF National Institute for Astrophysics, 36Technische Universität Dortmund, 37Universidad Complutense, 38Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 39Universität Würzburg, 40Università di Padova and INFN, 41Technische Universität Dortmund, 42Universität Würzburg, 43Technische Universität Dortmund, 44Technische Universität Dortmund, 45Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 46Institut de Fisica d'Altes Energies, 47Universidad Complutense, 48Universidad Complutense, 49Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, 50Technische Universität Dortmund, 51Max-Planck-Institut für Physik, 52Universitat de Barcelona, ICC, 53Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 54Deutsches Elektronen-Synchrotron, 55Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, 56Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, 57INAF National Institute for Astrophysics, 58Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 59Deutsches Elektronen-Synchrotron, 60Institut de Fisica d'Altes Energies, 61Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 62Max-Planck-Institut für Physik, 63Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 64Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 65Max-Planck-Institut für Physik, 66Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 67ETH Zurich, 68University of Łódź, 69Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 70Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 71Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 72Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 73INAF National Institute for Astrophysics, 74Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 75Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 76INAF National Institute for Astrophysics, 77Università di Udine, INFN Trieste, 78Universidad Complutense, 79Institut de Fisica d'Altes Energies, 80Saha Institute of Nuclear Physics, 1/AF Bidhannagar, 81Inst. for Nucl. Research and Nucl. Energy, 82Deutsches Elektronen-Synchrotron, 83Inst. for Nucl. Research and Nucl. Energy, 84Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 85Università di Udine, INFN Trieste, 86Universität Würzburg, 87INAF National Institute for Astrophysics, 88Universitat de Barcelona, ICC, 89Università di Padova and INFN, 90Institut de Fisica d'Altes Energies, 91Max-Planck-Institut für Physik, 92Max-Planck-Institut für Physik, 93Università di Siena, INFN Pisa, 94Max-Planck-Institut für Physik, 95Institut de Fisica d'Altes Energies, 96Max-Planck-Institut für Physik, 97Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 98Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 99University of Łódź, 100Universidad Complutense, 101Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 102Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 103Max-Planck-Institut für Physik, 104Institut de Fisica d'Altes Energies, 105Università di Padova and INFN, 106Institut de Fisica d'Altes Energies, 107Università di Udine, INFN Trieste, 108Max-Planck-Institut für Physik, 109Università di Siena, INFN Pisa, 110Universitat de Barcelona, ICC, 111Universitat de Barcelona, ICC, 112Deutsches Elektronen-Synchrotron, 113Università di Udine, INFN Trieste, 114INAF National Institute for Astrophysics, 115Università di Udine, INFN Trieste, 116Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 117Università di Pisa, and INFN Pisa, 118ETH Zurich, 119Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 120Max-Planck-Institut für Physik, 121Università di Padova and INFN, 122Technische Universität Dortmund, 123Universitat de Barcelona, ICC, 124Institut de Fisica d'Altes Energies, 125Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 126Deutsches Elektronen-Synchrotron, 127Technische Universität Dortmund, 128Max-Planck-Institut für Physik, 129Università di Pisa, and INFN Pisa, 130Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 131University of Łódź, 132Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 133University of Łódź, 134INAF National Institute for Astrophysics, 135Max-Planck-Institut für Physik, 136Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 137Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 138Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, 139INAF National Institute for Astrophysics, 140Inst. for Nucl. Research and Nucl. Energy, 141Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 142Università di Padova and INFN, 143Max-Planck-Institut für Physik, 144ICREA and Institute for Space Sciences, 145Max-Planck-Institut für Physik, 146Università di Udine, INFN Trieste, 147Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 148Inst. for Nucl. Research and Nucl. Energy, 149Max-Planck-Institut für Physik, 150Institut de Fisica d'Altes Energies, 151Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 152Institute for Space Sciences, 153Universitat de Barcelona, ICC, 154Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 155Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 156Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica, 157NASA Goddard Space Flight Center, 158GRAPPA and Anton Pannekoek Institute for Astronomy, University of Amsterdam, 159INAF National Institute for Astrophysics, 160INAF National Institute for Astrophysics, 161Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland

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. Read More

47 Tuc X9 is a low mass X-ray binary (LMXB) in the globular cluster 47 Tucanae, and was previously thought to be a cataclysmic variable. However, Miller-Jones et al. (2015) recently identified a radio counterpart to X9 (inferring a radio/X-ray luminosity ratio consistent with black hole LMXBs), and suggested that the donor star might be a white dwarf. Read More

We present a spectral analysis of the NuSTAR and XMM-Newton observations of the Seyfert 1h galaxy/ULIRG IRAS 05189-2524 taken in 2013. We find evidence for relativistic disk reflection in the broadband X-ray spectrum: a highly asymmetric broad Fe K$\alpha$ emission line extending down to 3 keV and a Compton scattering component above 10 keV. Physical modeling with a self-consistent disk reflection model suggests the accretion disk is viewed at an intermediate angle with a super-solar iron abundance, and a mild constraint can be put on the high-energy cutoff of the power-law continuum. Read More

Metasurfaces offer significant potential to control far-field light propagation through the engineering of amplitude, polarization, and phase at an interface. We report here phase modulation of an electronically reconfigurable metasurface and demonstrate its utility for mid-infrared beam steering. Using a gate-tunable graphene-gold resonator geometry, we demonstrate highly tunable reflected phase at multiple wavelengths and show up to 237{\deg} phase modulation range at an operating wavelength of 8. Read More

The polyol route is a versatile and up-scalable method to produce large batches of iron oxide nanoparticles with well-defined structure and magnetic properties. Controlling parameters such as temperature and duration of reaction, heating profile, nature of polyol solvent or of organometallic precursors were reported in previous studies of literature, but none of them described yet the crucial role of water in the forced hydrolysis pathway, whose presence is mandatory for nanoparticle production. This communication investigates the influence of the water amount and temperature at which it is injected in the reflux system for either pure polyol or mixture with a poly(hydroxy) amine. Read More

Continuum and reflection spectral models have each been widely employed in measuring the spins of accreting black holes. However, the two approaches have not been implemented together in a photon-conserving, self-consistent framework. We develop such a framework using the black-hole X-ray binary GX 339-4 as a touchstone source, and we demonstrate three important ramifications: (1) Compton scattering of reflection emission in the corona is routinely ignored, but is an essential consideration given that reflection is linked to the regimes with strongest Comptonization. Read More

MCG-5-23-16 was targeted in early 2015 with a half mega-seconds observing campaign using NuSTAR. Here we present the spectral analysis of these datasets along with an earlier observation and study the relativistic reflection and the primary coronal source. The data show strong reflection features in the form of both narrow and broad iron lines plus a Compton reflection hump. Read More

2016Dec
Authors: M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, P. Antoranz4, A. Babic5, B. Banerjee6, P. Bangale7, U. Barres de Almeida8, J. A. Barrio9, J. Becerra González10, W. Bednarek11, E. Bernardini12, A. Berti13, B. Biasuzzi14, A. Biland15, O. Blanch16, S. Bonnefoy17, G. Bonnoli18, F. Borracci19, T. Bretz20, S. Buson21, A. Carosi22, A. Chatterjee23, R. Clavero24, P. Colin25, E. Colombo26, J. L. Contreras27, J. Cortina28, S. Covino29, P. Da Vela30, F. Dazzi31, A. De Angelis32, B. De Lotto33, E. de Ona Wilhelmi34, F. Di Pierro35, M. Doert36, A. Domínguez37, D. Dominis Prester38, D. Dorner39, M. Doro40, S. Einecke41, D. Eisenacher Glawion42, D. Elsaesser43, M. Engelkemeier44, V. Fallah Ramazani45, A. Fernández-Barral46, D. Fidalgo47, M. V. Fonseca48, L. Font49, K. Frantzen50, C. Fruck51, D. Galindo52, R. J. García López53, M. Garczarczyk54, D. Garrido Terrats55, M. Gaug56, P. Giammaria57, N. Godinović58, A. González Munoz59, D. Gora60, D. Guberman61, D. Hadasch62, A. Hahn63, Y. Hanabata64, M. Hayashida65, J. Herrera66, J. Hose67, D. Hrupec68, G. Hughes69, W. Idec70, K. Kodani71, Y. Konno72, H. Kubo73, J. Kushida74, A. La Barbera75, D. Lelas76, E. Lindfors77, S. Lombardi78, F. Longo79, M. López80, R. López-Coto81, P. Majumdar82, M. Makariev83, K. Mallot84, G. Maneva85, M. Manganaro86, K. Mannheim87, L. Maraschi88, B. Marcote89, M. Mariotti90, M. Martínez91, D. Mazin92, U. Menzel93, J. M. Miranda94, R. Mirzoyan95, A. Moralejo96, E. Moretti97, D. Nakajima98, V. Neustroev99, A. Niedzwiecki100, M. Nievas Rosillo101, K. Nilsson102, K. Nishijima103, K. Noda104, L. Nogués105, A. Overkemping106, S. Paiano107, J. Palacio108, M. Palatiello109, D. Paneque110, R. Paoletti111, J. M. Paredes112, X. Paredes-Fortuny113, G. Pedaletti114, M. Peresano115, L. Perri116, M. Persic117, J. Poutanen118, P. G. Prada Moroni119, E. Prandini120, I. Puljak121, I. Reichardt122, W. Rhode123, M. Ribó124, J. Rico125, J. Rodriguez Garcia126, T. Saito127, K. Satalecka128, S. Schröder129, C. Schultz130, T. Schweizer131, S. N. Shore132, A. Sillanpää133, J. Sitarek134, I. Snidaric135, D. Sobczynska136, A. Stamerra137, T. Steinbring138, M. Strzys139, T. Surić140, L. Takalo141, F. Tavecchio142, P. Temnikov143, T. Terzić144, D. Tescaro145, M. Teshima146, J. Thaele147, D. F. Torres148, T. Toyama149, A. Treves150, G. Vanzo151, V. Verguilov152, I. Vovk153, J. E. Ward154, M. Will155, M. H. Wu156, R. Zanin157, A. U. Abeysekara158, S. Archambault159, A. Archer160, W. Benbow161, R. Bird162, M. Buchovecky163, J. H. Buckley164, V. Bugaev165, M. P. Connolly166, W. Cui167, H. J. Dickinson168, A. Falcone169, Q. Feng170, J. P. Finley171, H. Fleischhack172, A. Flinders173, L. Fortson174, G. H. Gillanders175, S. Griffin176, J. Grube177, M. Hütten178, D. Hanna179, J. Holder180, T. B. Humensky181, P. Kaaret182, P. Kar183, N. Kelley-Hoskins184, M. Kertzman185, D. Kieda186, M. Krause187, F. Krennrich188, M. J. Lang189, G. Maier190, A. McCann191, P. Moriarty192, R. Mukherjee193, D. Nieto194, S. O'Brien195, R. A. Ong196, N. Otte197, N. Park198, J. Perkins199, A. Pichel200, M. Pohl201, A. Popkow202, E. Pueschel203, J. Quinn204, K. Ragan205, P. T. Reynolds206, G. T. Richards207, E. Roache208, A. C. Rovero209, C. Rulten210, I. Sadeh211, M. Santander212, G. H. Sembroski213, K. Shahinyan214, I. Telezhinsky215, J. V. Tucci216, J. Tyler217, S. P. Wakely218, A. Weinstein219, P. Wilcox220, A. Wilhelm221, D. A. Williams222, B. Zitzer223, S. Razzaque224, M. Villata225, C. M. Raiteri226, H. D. Aller227, M. F. Aller228, V. M. Larionov229, A. A. Arkharov230, D. A. Blinov231, N. V. Efimova232, T. S. Grishina233, V. A. Hagen-Thorn234, E. N. Kopatskaya235, L. V. Larionova236, E. G. Larionova237, D. A. Morozova238, I. S. Troitsky239, R. Ligustri240, P. Calcidese241, A. Berdyugin242, O. M. Kurtanidze243, M. G. Nikolashvili244, G. N. Kimeridze245, L. A. Sigua246, S. O. Kurtanidze247, R. A. Chigladze248, W. P. Chen249, E. Koptelova250, T. Sakamoto251, A. C. Sadun252, J. W. Moody253, C. Pace254, R. Pearson III255, Y. Yatsu256, Y. Mori257, A. Carraminyana258, L. Carrasco259, E. de la Fuente260, J. P. Norris261, P. S. Smith262, A. Wehrle263, M. A. Gurwell264, Alma Zook265, C. Pagani266, M. Perri267, M. Capalbi268, A. Cesarini269, H. A. Krimm270, Y. Y. Kovalev271, Yu. A. Kovalev272, E. Ros273, A. B. Pushkarev274, M. L. Lister275, K. V. Sokolovsky276, M. Kadler277, G. Piner278, A. Lähteenmäki279, M. Tornikoski280, E. Angelakis281, T. P. Krichbaum282, I. Nestoras283, L Fuhrmann284, J. A. Zensus285, P. Cassaro286, A. Orlati287, G. Maccaferri288, P. Leto289, M. Giroletti290, J. L. Richards291, W. Max-Moerbeck292, A. C. S. Readhead293
Affiliations: 1ETH Zurich, Switzerland, 2Università di Udine, and INFN Trieste, Udine, Italy, 3INAF National Institute for Astrophysics, Rome, Italy, 4Università di Siena, and INFN Pisa, Siena, Italy, 5Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 6Saha Institute of Nuclear Physics, Kolkata, India, 7Max-Planck-Institut für Physik, München, Germany, 8Max-Planck-Institut für Physik, München, Germany, 9Universidad Complutense, Madrid, Spain, 10Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 11University of Łódź, Lodz, Poland, 12Deutsches Elektronen-Synchrotron, 13Università di Udine, and INFN Trieste, Udine, Italy, 14Università di Udine, and INFN Trieste, Udine, Italy, 15ETH Zurich, Switzerland, 16Institut de Fisica d'Altes Energies, 17Universidad Complutense, Madrid, Spain, 18INAF National Institute for Astrophysics, Rome, Italy, 19Max-Planck-Institut für Physik, München, Germany, 20Universität Würzburg, Würzburg, Germany, 21Università di Padova and INFN, Padova, Italy, 22INAF National Institute for Astrophysics, Rome, Italy, 23Saha Institute of Nuclear Physics, Kolkata, India, 24Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 25Max-Planck-Institut für Physik, München, Germany, 26Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 27Universidad Complutense, Madrid, Spain, 28Institut de Fisica d'Altes Energies, 29INAF National Institute for Astrophysics, Rome, Italy, 30Università di Siena, and INFN Pisa, Siena, Italy, 31Max-Planck-Institut für Physik, München, Germany, 32Università di Padova and INFN, Padova, Italy, 33Università di Udine, and INFN Trieste, Udine, Italy, 34Institute for Space Sciences, 35INAF National Institute for Astrophysics, Rome, Italy, 36Technische Universität Dortmund, Dortmund, Germany, 37Universidad Complutense, Madrid, Spain, 38Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 39Universität Würzburg, Würzburg, Germany, 40Università di Padova and INFN, Padova, Italy, 41Technische Universität Dortmund, Dortmund, Germany, 42Universität Würzburg, Würzburg, Germany, 43Technische Universität Dortmund, Dortmund, Germany, 44Technische Universität Dortmund, Dortmund, Germany, 45Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 46Institut de Fisica d'Altes Energies, 47Universidad Complutense, Madrid, Spain, 48Universidad Complutense, Madrid, Spain, 49Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Barcelona, Spain, 50Technische Universität Dortmund, Dortmund, Germany, 51Max-Planck-Institut für Physik, München, Germany, 52Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 53Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 54Deutsches Elektronen-Synchrotron, 55Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Barcelona, Spain, 56Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Barcelona, Spain, 57INAF National Institute for Astrophysics, Rome, Italy, 58Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 59Institut de Fisica d'Altes Energies, 60Deutsches Elektronen-Synchrotron, 61Institut de Fisica d'Altes Energies, 62Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 63Max-Planck-Institut für Physik, München, Germany, 64Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 65Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 66Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 67Max-Planck-Institut für Physik, München, Germany, 68Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 69ETH Zurich, Switzerland, 70University of Łódź, Lodz, Poland, 71Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 72Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 73Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 74Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 75INAF National Institute for Astrophysics, Rome, Italy, 76Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 77Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 78INAF National Institute for Astrophysics, Rome, Italy, 79Università di Udine, and INFN Trieste, Udine, Italy, 80Universidad Complutense, Madrid, Spain, 81Institut de Fisica d'Altes Energies, 82Saha Institute of Nuclear Physics, Kolkata, India, 83Inst. for Nucl. Research and Nucl. Energy, Sofia, Bulgaria, 84Deutsches Elektronen-Synchrotron, 85Inst. for Nucl. Research and Nucl. Energy, Sofia, Bulgaria, 86Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 87Universität Würzburg, Würzburg, Germany, 88INAF National Institute for Astrophysics, Rome, Italy, 89Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 90Università di Padova and INFN, Padova, Italy, 91Institut de Fisica d'Altes Energies, 92Max-Planck-Institut für Physik, München, Germany, 93Max-Planck-Institut für Physik, München, Germany, 94Università di Siena, and INFN Pisa, Siena, Italy, 95Max-Planck-Institut für Physik, München, Germany, 96Institut de Fisica d'Altes Energies, 97Max-Planck-Institut für Physik, München, Germany, 98Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 99Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 100University of Łódź, Lodz, Poland, 101Universidad Complutense, Madrid, Spain, 102Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 103Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 104Max-Planck-Institut für Physik, München, Germany, 105Institut de Fisica d'Altes Energies, 106Technische Universität Dortmund, Dortmund, Germany, 107Università di Padova and INFN, Padova, Italy, 108Institut de Fisica d'Altes Energies, 109Università di Udine, and INFN Trieste, Udine, Italy, 110Max-Planck-Institut für Physik, München, Germany, 111Università di Siena, and INFN Pisa, Siena, Italy, 112Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 113Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 114Deutsches Elektronen-Synchrotron, 115Università di Udine, and INFN Trieste, Udine, Italy, 116INAF National Institute for Astrophysics, Rome, Italy, 117Università di Udine, and INFN Trieste, Udine, Italy, 118Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 119Università di Pisa, and INFN Pisa, Pisa, Italy, 120ETH Zurich, Switzerland, 121Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 122Università di Padova and INFN, Padova, Italy, 123Technische Universität Dortmund, Dortmund, Germany, 124Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 125Institut de Fisica d'Altes Energies, 126Max-Planck-Institut für Physik, München, Germany, 127Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 128Deutsches Elektronen-Synchrotron, 129Technische Universität Dortmund, Dortmund, Germany, 130Università di Padova and INFN, Padova, Italy, 131Max-Planck-Institut für Physik, München, Germany, 132Università di Pisa, and INFN Pisa, Pisa, Italy, 133Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 134University of Łódź, Lodz, Poland, 135Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 136University of Łódź, Lodz, Poland, 137INAF National Institute for Astrophysics, Rome, Italy, 138Universität Würzburg, Würzburg, Germany, 139Max-Planck-Institut für Physik, München, Germany, 140Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 141Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 142INAF National Institute for Astrophysics, Rome, Italy, 143Inst. for Nucl. Research and Nucl. Energy, Sofia, Bulgaria, 144Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 145Università di Padova and INFN, Padova, Italy, 146Max-Planck-Institut für Physik, München, Germany, 147Technische Universität Dortmund, Dortmund, Germany, 148ICREA and Institute for Space Sciences, 149Max-Planck-Institut für Physik, München, Germany, 150Università di Udine, and INFN Trieste, Udine, Italy, 151Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 152Inst. for Nucl. Research and Nucl. Energy, Sofia, Bulgaria, 153Max-Planck-Institut für Physik, München, Germany, 154Institut de Fisica d'Altes Energies, 155Inst. de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, Tenerife, Spain, 156Institute for Space Sciences, 157Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 158Department of Physics and Astronomy, University of Utah, Salt Lake City, USA, 159Physics Department, McGill University, Montreal, Canada, 160Department of Physics, Washington University, St. Louis, USA, 161Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, USA, 162School of Physics, University College Dublin, Belfield, Ireland, 163Department of Physics and Astronomy, University of California, Los Angeles, USA, 164Department of Physics, Washington University, St. Louis, USA, 165Department of Physics, Washington University, St. Louis, USA, 166School of Physics, National University of Ireland Galway, Galway, Ireland, 167Department of Physics and Astronomy, Purdue University, West Lafayette, USA, 168Department of Physics and Astronomy, Iowa State University, Ames, USA, 169Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, USA, 170Department of Physics and Astronomy, Purdue University, West Lafayette, USA, 171Department of Physics and Astronomy, Purdue University, West Lafayette, USA, 172Deutsches Elektronen-Synchrotron, 173Department of Physics and Astronomy, University of Utah, Salt Lake City, USA, 174School of Physics and Astronomy, University of Minnesota, Minneapolis, USA, 175School of Physics, National University of Ireland Galway, Galway, Ireland, 176Physics Department, McGill University, Montreal, Canada, 177Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, USA, 178Deutsches Elektronen-Synchrotron, 179Physics Department, McGill University, Montreal, Canada, 180Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, USA, 181Physics Department, Columbia University, New York, USA, 182Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, USA, 183Department of Physics and Astronomy, University of Utah, Salt Lake City, USA, 184Deutsches Elektronen-Synchrotron, 185Department of Physics and Astronomy, DePauw University, Greencastle, USA, 186Department of Physics and Astronomy, University of Utah, Salt Lake City, USA, 187Deutsches Elektronen-Synchrotron, 188Department of Physics and Astronomy, Iowa State University, Ames, USA, 189School of Physics, National University of Ireland Galway, Galway, Ireland, 190Deutsches Elektronen-Synchrotron, 191Physics Department, McGill University, Montreal, Canada, 192School of Physics, National University of Ireland Galway, Galway, Ireland, 193Department of Physics and Astronomy, Barnard College, Columbia University, USA, 194Physics Department, Columbia University, New York, USA, 195School of Physics, University College Dublin, Belfield, Ireland, 196Department of Physics and Astronomy, University of California, Los Angeles, USA, 197School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, USA, 198Enrico Fermi Institute, University of Chicago, Chicago, USA, 199NASA Goddard Space Flight Center, Greenbelt, USA, 200Instituto de Astronomia y Fisica del Espacio, Ciudad Automa de Buenos Aires, Argentina, 201Institute of Physics and Astronomy, University of Potsdam, Potsdam-Golm, Germany, 202Department of Physics and Astronomy, University of California, Los Angeles, USA, 203School of Physics, University College Dublin, Belfield, Ireland, 204School of Physics, University College Dublin, Belfield, Ireland, 205Physics Department, McGill University, Montreal, Canada, 206Department of Physical Sciences, Cork Institute of Technology, Bishopstown, Cork, Ireland, 207School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, USA, 208Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, USA, 209Instituto de Astronomia y Fisica del Espacio, Ciudad Automa de Buenos Aires, Argentina, 210School of Physics and Astronomy, University of Minnesota, Minneapolis, USA, 211Deutsches Elektronen-Synchrotron, 212Department of Physics and Astronomy, Barnard College, Columbia University, USA, 213Department of Physics and Astronomy, Purdue University, West Lafayette, USA, 214School of Physics and Astronomy, University of Minnesota, Minneapolis, USA, 215Institute of Physics and Astronomy, University of Potsdam, Potsdam-Golm, Germany, 216Department of Physics and Astronomy, Purdue University, West Lafayette, USA, 217Physics Department, McGill University, Montreal, Canada, 218Enrico Fermi Institute, University of Chicago, Chicago, USA, 219Department of Physics and Astronomy, Iowa State University, Ames, USA, 220Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, USA, 221Institute of Physics and Astronomy, University of Potsdam, Potsdam-Golm, Germany, 222Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, USA, 223Argonne National Laboratory, Argonne, USA, 224Department of Physics, University of Johannesburg, South Africa, 225INAF-Osservatorio Astrofisico di Torino, Torino, Italy, 226INAF-Osservatorio Astrofisico di Torino, Torino, Italy, 227Department of Astronomy, University of Michigan, Ann Arbor, USA, 228Department of Astronomy, University of Michigan, Ann Arbor, USA, 229Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 230Pulkovo Observatory, St.-Petersburg, Russia, 231Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 232Pulkovo Observatory, St.-Petersburg, Russia, 233Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 234Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 235Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 236Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 237Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 238Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 239Astronomical Institute, St. Petersburg State University, St. Petersburg, Russia, 240Circolo Astrofili Talmassons, Campoformido, Italy, 241Osservatorio Astrofisico della Regione Autonoma Valle d'Aosta, Italy, 242Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 243Abastumani Observatory, Abastumani, Georgia, 244Abastumani Observatory, Abastumani, Georgia, 245Abastumani Observatory, Abastumani, Georgia, 246Abastumani Observatory, Abastumani, Georgia, 247Abastumani Observatory, Abastumani, Georgia, 248Abastumani Observatory, Abastumani, Georgia, 249Graduate Institute of Astronomy, National Central University, Zhongli, Taiwan, 250Graduate Institute of Astronomy, National Central University, Zhongli, Taiwan, 251Department of Physics and Mathematics, College of Science and 952 Engineering, Aoyama Gakuin University, Sagamihara-shi Kanagawa, Japan, 252Department of Physics, University of Colorado Denver, Denver, Colorado, USA, 253Department of Physics and Astronomy, Brigham Young University, Provo, Utah, USA, 254Department of Physics and Astronomy, Brigham Young University, Provo, Utah, USA, 255Department of Physics and Astronomy, Brigham Young University, Provo, Utah, USA, 256Department of Physics, Tokyo Institute of Technology, Meguro City, Japan, 257Department of Physics, Tokyo Institute of Technology, Meguro City, Japan, 258Instituto Nacional de Astrofísica, Óptica y Electrónica, Tonantzintla, Puebla, Mexico, 259Instituto Nacional de Astrofísica, Óptica y Electrónica, Tonantzintla, Puebla, Mexico, 260Instututo de Astronomia y Meteorologia, Dpto. de Fisica, CUCEI, Universidad de Guadalajara, 261Department of Physics and Astronomy, University of Denver, Denver, USA, 262Steward Observatory, University of Arizona, Tucson, USA, 263Space Science Institute, Boulder, USA, 264Harvard-Smithsonian Center for Astrophysics, Cambridge, USA, 265Department of Physics and Astronomy, Pomona College, Claremont, USA, 266Department of Physics and Astronomy, University of Leicester, Leicester, UK, 267ASI Science Data Center, Via del Politecnico, Roma, Italy, 268ASI Science Data Center, Via del Politecnico, Roma, Italy, 269Department of Physics, University of Trento, Trento, Italy, 270NASA Goddard Space Flight Center, Greenbelt, USA, 271Astro Space Center of Lebedev Physical Institute, Moscow, Russia, 272Astro Space Center of Lebedev Physical Institute, Moscow, Russia, 273Max-Planck-Institut für Radioastronomie, Bonn, Germany, 274Astro Space Center of Lebedev Physical Institute, Moscow, Russia, 275Department of Physics and Astronomy, Purdue University, West Lafayette, USA, 276Astro Space Center of Lebedev Physical Institute, Moscow, Russia, 277Universität Würzburg, Würzburg, Germany, 278Department of Physics and Astronomy, Whittier College, Whittier, USA, 279Aalto University Metsähovi Radio Observatory, Finland, 280Aalto University Metsähovi Radio Observatory, Finland, 281Max-Planck-Institut für Radioastronomie, Bonn, Germany, 282Max-Planck-Institut für Radioastronomie, Bonn, Germany, 283Max-Planck-Institut für Radioastronomie, Bonn, Germany, 284Max-Planck-Institut für Radioastronomie, Bonn, Germany, 285Max-Planck-Institut für Radioastronomie, Bonn, Germany, 286INAF Istituto di Radioastronomia, Sezione di Noto, Noto, Italy, 287INAF Istituto di Radioastronomia, Stazione Radioastronomica di Medicina, Medicina Bologna, Italy, 288INAF Istituto di Radioastronomia, Stazione Radioastronomica di Medicina, Medicina Bologna, Italy, 289INAF Osservatorio Astrofisico di Catania, Catania, Italy, 290INAF Istituto di Radioastronomia, Stazione Radioastronomica di Medicina, Medicina Bologna, Italy, 291Department of Physics and Astronomy, Purdue University, West Lafayette, USA, 292Max-Planck-Institut für Radioastronomie, Bonn, Germany, 293Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, USA

We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1 which includes, among other instruments, MAGIC, VERITAS, Whipple 10-m, Fermi-LAT, RXTE, Swift, GASP-WEBT and VLBA. We find an increase in the fractional variability with energy, while no significant interband correlations of flux changes are found in the acquired data set. The higher variability in the very high energy (>100 GeV, VHE) gamma-ray emission and the lack of correlation with the X-ray emission indicate that the highest-energy electrons that are responsible for the VHE gamma-rays do not make a dominant contribution to the ~1 keV emission. Read More

In recent years governments have shown themselves willing to impose blackouts to shut off key communication infrastructure during times of civil strife, and to surveil citizen communications whenever possible. However, it is exactly during such strife that citizens need reliable and anonymous communications the most. In this paper, we present Rangzen, a system for anonymous broadcast messaging during network blackouts. Read More

In this work, we consider a STU black-hole model containing eight magnetic and eight electric charges ((8+8)-signature). We show that such model admits an extremal black holes solution in which (8+8)-signature can be associated with the entropy via the Cayley's hyperdeterminant. Read More

2016Dec
Affiliations: 1SPINTEC - UMR 8191, 2SPINTEC - UMR 8191, 3SPINTEC - UMR 8191, 4IBM Research Laboratory Zurich, 5IBM Research Laboratory Zurich, 6IBM Research Laboratory Zurich, 7IBM Research Laboratory Zurich, 8SPINTEC - UMR 8191, 9SPINTEC - UMR 8191, 10SPINTEC - UMR 8191, 11SPINTEC - UMR 8191, 12SPINTEC - UMR 8191, 13SPINTEC - UMR 8191

Segmented magnetic nanowires are a promising route for the development of three dimensional data storage techniques. Such devices require a control of the coercive field and the coupling mechanisms between individual magnetic elements. In our study, we investigate electrodeposited nanomagnets within host templates using vibrating sample magnetometry and observe a strong dependence between nanowire length and coercive field (25 nm to 5 $\mu$m) and diameter (25 nm to 45 nm). Read More

2016Nov
Authors: M. L. Ahnen, S. Ansoldi, L. A. Antonelli, P. Antoranz, C. Arcaro, A. Babic, B. Banerjee, P. Bangale, U. Barres de Almeida, J. A. Barrio, J. Becerra González, W. Bednarek, E. Bernardini, A. Berti, B. Biasuzzi, A. Biland, O. Blanch, S. Bonnefoy, G. Bonnoli, F. Borracci, T. Bretz, S. Buson, A. Carosi, A. Chatterjee, R. Clavero, P. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, E. de Oña Wilhelmi, F. Di Pierro, M. Doert, A. Domínguez, D. Dominis Prester, D. Dorner, M. Doro, S. Einecke, D. Eisenacher Glawion, D. Elsaesser, M. Engelkemeier, V. Fallah Ramazani, A. Fernández-Barral, D. Fidalgo, M. V. Fonseca, L. Font, K. Frantzen, C. Fruck, D. Galindo, R. J. García López, M. Garczarczyk, D. Garrido Terrats, M. Gaug, P. Giammaria, N. Godinović, A. González Muñoz, D. Gora, D. Guberman, D. Hadasch, A. Hahn, M. Hayashida, J. Herrera, J. Hose, D. Hrupec, G. Hughes, W. Idec, K. Kodani, Y. Konno, H. Kubo, J. Kushida, A. La Barbera, D. Lelas, E. Lindfors, S. Lombardi, F. Longo, M. López, R. López-Coto, P. Majumdar, M. Makariev, K. Mallot, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, B. Marcote, M. Mariotti, M. Martínez, D. Mazin, U. Menzel, J. M. Miranda, R. Mirzoyan, A. Moralejo, E. Moretti, D. Nakajima, V. Neustroev, A. Niedzwiecki, M. Nievas Rosillo, K. Nilsson, K. Nishijima, K. Noda, L. Nogués, A. Overkemping, S. Paiano, J. Palacio, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, X. Paredes-Fortuny, G. Pedaletti, M. Peresano, L. Perri, M. Persic, J. Poutanen, P. G. Prada Moroni, E. Prandini, I. Puljak, J. R. Garcia, I. Reichardt, W. Rhode, M. Ribó, J. Rico, T. Saito, K. Satalecka, S. Schroeder, T. Schweizer, S. N. Shore, A. Sillanpää, J. Sitarek, I. Snidaric, D. Sobczynska, A. Stamerra, T. Steinbring, M. Strzys, T. Surić, L. Takalo, F. Tavecchio, P. Temnikov, T. Terzić, D. Tescaro, M. Teshima, J. Thaele, D. F. Torres, T. Toyama, A. Treves, G. Vanzo, V. Verguilov, I. Vovk, J. E. Ward, M. Will, M. H. Wu, R. Zanin

Context. We present the results of a multi-year monitoring campaign of the Galactic Center (GC) with the MAGIC telescopes. These observations were primarily motivated by reports that a putative gas cloud (G2) would be passing in close proximity to the super-massive black hole (SMBH), associated with Sagittarius A*, located at the center of our galaxy. Read More

2016Nov
Authors: A. U. Abeysekara1, S. Archambault2, A. Archer3, W. Benbow4, R. Bird5, M. Buchovecky6, J. H. Buckley7, V. Bugaev8, J. V Cardenzana9, M. Cerruti10, X. Chen11, L. Ciupik12, M. P. Connolly13, W. Cui14, J. D. Eisch15, A. Falcone16, Q. Feng17, J. P. Finley18, H. Fleischhack19, A. Flinders20, L. Fortson21, A. Furniss22, S. Griffin23, M. Hütten24, N. Håkansson25, D. Hanna26, O. Hervet27, J. Holder28, T. B. Humensky29, P. Kaaret30, P. Kar31, M. Kertzman32, D. Kieda33, M. Krause34, S. Kumar35, M. J. Lang36, G. Maier37, S. McArthur38, A. McCann39, K. Meagher40, P. Moriarty41, R. Mukherjee42, D. Nieto43, S. O'Brien44, R. A. Ong45, A. N. Otte46, N. Park47, V. Pelassa48, M. Pohl49, A. Popkow50, E. Pueschel51, K. Ragan52, P. T. Reynolds53, G. T. Richards54, E. Roache55, I. Sadeh56, M. Santander57, G. H. Sembroski58, K. Shahinyan59, D. Staszak60, I. Telezhinsky61, J. V. Tucci62, J. Tyler63, S. P. Wakely64, A. Weinstein65, A. Wilhelm66, D. A. Williams67, M. L. Ahnen68, S. Ansoldi69, L. A. Antonelli70, P. Antoranz71, C. Arcaro72, A. Babic73, B. Banerjee74, P. Bangale75, U. Barres de Almeida76, J. A. Barrio77, J. Becerra González78, W. Bednarek79, E. Bernardini80, A. Berti81, B. Biasuzzi82, A. Biland83, O. Blanch84, S. Bonnefoy85, G. Bonnoli86, F. Borracci87, T. Bretz88, R. Carosi89, A. Carosi90, A. Chatterjee91, P. Colin92, E. Colombo93, J. L. Contreras94, J. Cortina95, S. Covino96, P. Cumani97, P. Da Vela98, F. Dazzi99, A. De Angelis100, B. De Lotto101, E. de Oña Wilhelmi102, F. Di Pierro103, M. Doert104, A. Domínguez105, D. Dominis Prester106, D. Dorner107, M. Doro108, S. Einecke109, D. Eisenacher Glawion110, D. Elsaesser111, M. Engelkemeier112, V. Fallah Ramazani113, A. Fernández-Barral114, D. Fidalgo115, M. V. Fonseca116, L. Font117, C. Fruck118, D. Galindo119, R. J. García López120, M. Garczarczyk121, M. Gaug122, P. Giammaria123, N. Godinović124, D. Gora125, D. Guberman126, D. Hadasch127, A. Hahn128, T. Hassan129, M. Hayashida130, J. Herrera131, J. Hose132, D. Hrupec133, G. Hughes134, W. Idec135, K. Kodani136, Y. Konno137, H. Kubo138, J. Kushida139, D. Lelas140, E. Lindfors141, S. Lombardi142, F. Longo143, M. López144, R. López-Coto145, P. Majumdar146, M. Makariev147, K. Mallot148, G. Maneva149, M. Manganaro150, K. Mannheim151, L. Maraschi152, B. Marcote153, M. Mariotti154, M. Martínez155, D. Mazin156, U. Menzel157, R. Mirzoyan158, A. Moralejo159, E. Moretti160, D. Nakajima161, V. Neustroev162, A. Niedzwiecki163, M. Nievas Rosillo164, K. Nilsson165, K. Nishijima166, K. Noda167, L. Nogués168, M. Nöthe169, S. Paiano170, J. Palacio171, M. Palatiello172, D. Paneque173, R. Paoletti174, J. M. Paredes175, X. Paredes-Fortuny176, G. Pedaletti177, M. Peresano178, L. Perri179, M. Persic180, J. Poutanen181, P. G. Prada Moroni182, E. Prandini183, I. Puljak184, J. R. Garcia185, I. Reichardt186, W. Rhode187, M. Ribó188, J. Rico189, T. Saito190, K. Satalecka191, S. Schroeder192, T. Schweizer193, S. N. Shore194, A. Sillanpää195, J. Sitarek196, I. Snidaric197, D. Sobczynska198, A. Stamerra199, M. Strzys200, T. Surić201, L. Takalo202, F. Tavecchio203, P. Temnikov204, T. Terzić205, D. Tescaro206, M. Teshima207, D. F. Torres208, N. Torres-Albà209, T. Toyama210, A. Treves211, G. Vanzo212, M. Vazquez Acosta213, I. Vovk214, J. E. Ward215, M. Will216, M. H. Wu217, R. Zanin218, T. Hovatta, I. de la Calle Perez, P. S. Smith, E. Racero, M. Baloković
Affiliations: 1the VERITAS Collaboration, 2the VERITAS Collaboration, 3the VERITAS Collaboration, 4the VERITAS Collaboration, 5the VERITAS Collaboration, 6the VERITAS Collaboration, 7the VERITAS Collaboration, 8the VERITAS Collaboration, 9the VERITAS Collaboration, 10the VERITAS Collaboration, 11the VERITAS Collaboration, 12the VERITAS Collaboration, 13the VERITAS Collaboration, 14the VERITAS Collaboration, 15the VERITAS Collaboration, 16the VERITAS Collaboration, 17the VERITAS Collaboration, 18the VERITAS Collaboration, 19the VERITAS Collaboration, 20the VERITAS Collaboration, 21the VERITAS Collaboration, 22the VERITAS Collaboration, 23the VERITAS Collaboration, 24the VERITAS Collaboration, 25the VERITAS Collaboration, 26the VERITAS Collaboration, 27the VERITAS Collaboration, 28the VERITAS Collaboration, 29the VERITAS Collaboration, 30the VERITAS Collaboration, 31the VERITAS Collaboration, 32the VERITAS Collaboration, 33the VERITAS Collaboration, 34the VERITAS Collaboration, 35the VERITAS Collaboration, 36the VERITAS Collaboration, 37the VERITAS Collaboration, 38the VERITAS Collaboration, 39the VERITAS Collaboration, 40the VERITAS Collaboration, 41the VERITAS Collaboration, 42the VERITAS Collaboration, 43the VERITAS Collaboration, 44the VERITAS Collaboration, 45the VERITAS Collaboration, 46the VERITAS Collaboration, 47the VERITAS Collaboration, 48the VERITAS Collaboration, 49the VERITAS Collaboration, 50the VERITAS Collaboration, 51the VERITAS Collaboration, 52the VERITAS Collaboration, 53the VERITAS Collaboration, 54the VERITAS Collaboration, 55the VERITAS Collaboration, 56the VERITAS Collaboration, 57the VERITAS Collaboration, 58the VERITAS Collaboration, 59the VERITAS Collaboration, 60the VERITAS Collaboration, 61the VERITAS Collaboration, 62the VERITAS Collaboration, 63the VERITAS Collaboration, 64the VERITAS Collaboration, 65the VERITAS Collaboration, 66the VERITAS Collaboration, 67the VERITAS Collaboration, 68the MAGIC Collaboration, 69the MAGIC Collaboration, 70the MAGIC Collaboration, 71the MAGIC Collaboration, 72the MAGIC Collaboration, 73the MAGIC Collaboration, 74the MAGIC Collaboration, 75the MAGIC Collaboration, 76the MAGIC Collaboration, 77the MAGIC Collaboration, 78the MAGIC Collaboration, 79the MAGIC Collaboration, 80the MAGIC Collaboration, 81the MAGIC Collaboration, 82the MAGIC Collaboration, 83the MAGIC Collaboration, 84the MAGIC Collaboration, 85the MAGIC Collaboration, 86the MAGIC Collaboration, 87the MAGIC Collaboration, 88the MAGIC Collaboration, 89the MAGIC Collaboration, 90the MAGIC Collaboration, 91the MAGIC Collaboration, 92the MAGIC Collaboration, 93the MAGIC Collaboration, 94the MAGIC Collaboration, 95the MAGIC Collaboration, 96the MAGIC Collaboration, 97the MAGIC Collaboration, 98the MAGIC Collaboration, 99the MAGIC Collaboration, 100the MAGIC Collaboration, 101the MAGIC Collaboration, 102the MAGIC Collaboration, 103the MAGIC Collaboration, 104the MAGIC Collaboration, 105the MAGIC Collaboration, 106the MAGIC Collaboration, 107the MAGIC Collaboration, 108the MAGIC Collaboration, 109the MAGIC Collaboration, 110the MAGIC Collaboration, 111the MAGIC Collaboration, 112the MAGIC Collaboration, 113the MAGIC Collaboration, 114the MAGIC Collaboration, 115the MAGIC Collaboration, 116the MAGIC Collaboration, 117the MAGIC Collaboration, 118the MAGIC Collaboration, 119the MAGIC Collaboration, 120the MAGIC Collaboration, 121the MAGIC Collaboration, 122the MAGIC Collaboration, 123the MAGIC Collaboration, 124the MAGIC Collaboration, 125the MAGIC Collaboration, 126the MAGIC Collaboration, 127the MAGIC Collaboration, 128the MAGIC Collaboration, 129the MAGIC Collaboration, 130the MAGIC Collaboration, 131the MAGIC Collaboration, 132the MAGIC Collaboration, 133the MAGIC Collaboration, 134the MAGIC Collaboration, 135the MAGIC Collaboration, 136the MAGIC Collaboration, 137the MAGIC Collaboration, 138the MAGIC Collaboration, 139the MAGIC Collaboration, 140the MAGIC Collaboration, 141the MAGIC Collaboration, 142the MAGIC Collaboration, 143the MAGIC Collaboration, 144the MAGIC Collaboration, 145the MAGIC Collaboration, 146the MAGIC Collaboration, 147the MAGIC Collaboration, 148the MAGIC Collaboration, 149the MAGIC Collaboration, 150the MAGIC Collaboration, 151the MAGIC Collaboration, 152the MAGIC Collaboration, 153the MAGIC Collaboration, 154the MAGIC Collaboration, 155the MAGIC Collaboration, 156the MAGIC Collaboration, 157the MAGIC Collaboration, 158the MAGIC Collaboration, 159the MAGIC Collaboration, 160the MAGIC Collaboration, 161the MAGIC Collaboration, 162the MAGIC Collaboration, 163the MAGIC Collaboration, 164the MAGIC Collaboration, 165the MAGIC Collaboration, 166the MAGIC Collaboration, 167the MAGIC Collaboration, 168the MAGIC Collaboration, 169the MAGIC Collaboration, 170the MAGIC Collaboration, 171the MAGIC Collaboration, 172the MAGIC Collaboration, 173the MAGIC Collaboration, 174the MAGIC Collaboration, 175the MAGIC Collaboration, 176the MAGIC Collaboration, 177the MAGIC Collaboration, 178the MAGIC Collaboration, 179the MAGIC Collaboration, 180the MAGIC Collaboration, 181the MAGIC Collaboration, 182the MAGIC Collaboration, 183the MAGIC Collaboration, 184the MAGIC Collaboration, 185the MAGIC Collaboration, 186the MAGIC Collaboration, 187the MAGIC Collaboration, 188the MAGIC Collaboration, 189the MAGIC Collaboration, 190the MAGIC Collaboration, 191the MAGIC Collaboration, 192the MAGIC Collaboration, 193the MAGIC Collaboration, 194the MAGIC Collaboration, 195the MAGIC Collaboration, 196the MAGIC Collaboration, 197the MAGIC Collaboration, 198the MAGIC Collaboration, 199the MAGIC Collaboration, 200the MAGIC Collaboration, 201the MAGIC Collaboration, 202the MAGIC Collaboration, 203the MAGIC Collaboration, 204the MAGIC Collaboration, 205the MAGIC Collaboration, 206the MAGIC Collaboration, 207the MAGIC Collaboration, 208the MAGIC Collaboration, 209the MAGIC Collaboration, 210the MAGIC Collaboration, 211the MAGIC Collaboration, 212the MAGIC Collaboration, 213the MAGIC Collaboration, 214the MAGIC Collaboration, 215the MAGIC Collaboration, 216the MAGIC Collaboration, 217the MAGIC Collaboration, 218the MAGIC Collaboration

Blazars are variable emitters across all wavelengths over a wide range of timescales, from months down to minutes. It is therefore essential to observe blazars simultaneously at different wavelengths, especially in the X-ray and gamma-ray bands, where the broadband spectral energy distributions usually peak. In this work, we report on three "target-of-opportunity" (ToO) observations of Mrk 421, one of the brightest TeV blazars, triggered by a strong flaring event at TeV energies in 2014. Read More

The discovery of the integer quantum Hall effect in the early eighties of the last century, with highly precise quantization values for the Hall conductance in multiples of $e^2/h$, has been the first fascinating manifestation of the topological state of matter driven by magnetic field and disorder, and related to the formation of non-dissipative current flow. In 2005, several new phenomena such as the spin Hall effect and the quantum spin Hall effect were predicted in the presence of strong spin-orbit coupling and vanishing external magnetic field. More recently, the Zeeman spin Hall effect and the formation of valley Hall topological currents have been introduced for graphene-based systems, under time-reversal or inversion symmetry-breaking conditions, respectively. Read More

2016Oct
Authors: MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, C. Arcaro4, A. Babić5, B. Banerjee6, P. Bangale7, U. Barres de Almeida8, J. A. Barrio9, J. Becerra González10, W. Bednarek11, E. Bernardini12, A. Berti13, B. Biasuzzi14, A. Biland15, O. Blanch16, S. Bonnefoy17, G. Bonnoli18, F. Borracci19, T. Bretz20, R. Carosi21, A. Carosi22, A. Chatterjee23, P. Colin24, E. Colombo25, J. L. Contreras26, J. Cortina27, S. Covino28, P. Cumani29, P. Da Vela30, F. Dazzi31, A. De Angelis32, B. De Lotto33, E. de Oña Wilhelmi34, F. Di Pierro35, M. Doert36, A. Domínguez37, D. Dominis Prester38, D. Dorner39, M. Doro40, S. Einecke41, D. Eisenacher Glawion42, D. Elsaesser43, M. Engelkemeier44, V. Fallah Ramazani45, A. Fernández-Barral46, D. Fidalgo47, M. V. Fonseca48, L. Font49, C. Fruck50, D. Galindo51, R. J. García López52, M. Garczarczyk53, M. Gaug54, P. Giammaria55, N. Godinović56, D. Gora57, D. Guberman58, D. Hadasch59, A. Hahn60, T. Hassan61, M. Hayashida62, J. Herrera63, J. Hose64, D. Hrupec65, G. Hughes66, K. Ishio67, Y. Konno68, H. Kubo69, J. Kushida70, D. Kuveždić71, D. Lelas72, E. Lindfors73, S. Lombardi74, F. Longo75, M. López76, P. Majumdar77, M. Makariev78, G. Maneva79, M. Manganaro80, K. Mannheim81, L. Maraschi82, M. Mariotti83, M. Martínez84, D. Mazin85, U. Menzel86, R. Mirzoyan87, A. Moralejo88, E. Moretti89, D. Nakajima90, V. Neustroev91, A. Niedzwiecki92, M. Nievas Rosillo93, K. Nilsson94, K. Nishijima95, K. Noda96, L. Nogués97, S. Paiano98, J. Palacio99, M. Palatiello100, D. Paneque101, R. Paoletti102, J. M. Paredes103, X. Paredes-Fortuny104, G. Pedaletti105, M. Peresano106, L. Perri107, M. Persic108, J. Poutanen109, P. G. Prada Moroni110, E. Prandini111, I. Puljak112, J. R. Garcia113, I. Reichardt114, W. Rhode115, M. Ribó116, J. Rico117, T. Saito118, K. Satalecka119, S. Schroeder120, T. Schweizer121, S. N. Shore122, A. Sillanpää123, J. Sitarek124, I. Šnidarić125, D. Sobczynska126, A. Stamerra127, M. Strzys128, T. Surić129, L. Takalo130, F. Tavecchio131, P. Temnikov132, T. Terzić133, D. Tescaro134, M. Teshima135, D. F. Torres136, N. Torres-Albà137, T. Toyama138, A. Treves139, G. Vanzo140, M. Vazquez Acosta141, I. Vovk142, J. E. Ward143, M. Will144, M. H. Wu145, D. Zarić146, R. Desiante147, J. Becerra González148, F. D'Ammando149, S. Larsson150, C. M. Raiteri151, R. Reinthal152, A. Lähteenmäki153, E. Järvelä154, M. Tornikoski155, V. Ramakrishnan156, S. G. Jorstad157, A. P. Marscher158, V. Bala159, N. R. MacDonald160, N. Kaur161, Sameer162, K. Baliyan163, J. A. Acosta-Pulido164, C. Lazaro165, C. Martínez-Lombilla166, A. B. Grinon-Marin167, A. Pastor Yabar168, C. Protasio169, M. I. Carnerero170, H. Jermak171, I. A. Steele172, V. M. Larionov173, G. A. Borman174, T. S. Grishina175
Affiliations: 1ETH Zurich, Switzerland, 2Università di Udine, and INFN Trieste, Udine, Italy, 3INAF National Institute for Astrophysics, Rome, Italy, 4Università di Padova and INFN, Padova, Italy, 5Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 6Saha Institute of Nuclear Physics, Kolkata, India, 7Max-Planck-Institut für Physik, München, Germany, 8Max-Planck-Institut für Physik, München, Germany, 9Universidad Complutense, Madrid, Spain, 10Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 11University of Łódź, Lodz, Poland, 12Deutsches Elektronen-Synchrotron, 13Università di Udine, and INFN Trieste, Udine, Italy, 14Università di Udine, and INFN Trieste, Udine, Italy, 15ETH Zurich, Switzerland, 16Institut de Fisica d'Altes Energies, 17Universidad Complutense, Madrid, Spain, 18Università di Siena, and INFN Pisa, Siena, Italy, 19Max-Planck-Institut für Physik, München, Germany, 20Universität Würzburg, Würzburg, Germany, 21Università di Siena, and INFN Pisa, Siena, Italy, 22INAF National Institute for Astrophysics, Rome, Italy, 23Saha Institute of Nuclear Physics, Kolkata, India, 24Max-Planck-Institut für Physik, München, Germany, 25Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 26Universidad Complutense, Madrid, Spain, 27Institut de Fisica d'Altes Energies, 28INAF National Institute for Astrophysics, Rome, Italy, 29Institut de Fisica d'Altes Energies, 30Università di Siena, and INFN Pisa, Siena, Italy, 31Max-Planck-Institut für Physik, München, Germany, 32Università di Padova and INFN, Padova, Italy, 33Università di Udine, and INFN Trieste, Udine, Italy, 34Institute for Space Sciences, 35INAF National Institute for Astrophysics, Rome, Italy, 36Technische Universität Dortmund, Dortmund, Germany, 37Universidad Complutense, Madrid, Spain, 38Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 39Universität Würzburg, Würzburg, Germany, 40Università di Padova and INFN, Padova, Italy, 41Technische Universität Dortmund, Dortmund, Germany, 42Universität Würzburg, Würzburg, Germany, 43Technische Universität Dortmund, Dortmund, Germany, 44Technische Universität Dortmund, Dortmund, Germany, 45Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 46Institut de Fisica d'Altes Energies, 47Universidad Complutense, Madrid, Spain, 48Universidad Complutense, Madrid, Spain, 49Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Bellaterra, Spain, 50Max-Planck-Institut für Physik, München, Germany, 51Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 52Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 53Deutsches Elektronen-Synchrotron, 54Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Bellaterra, Spain, 55INAF National Institute for Astrophysics, Rome, Italy, 56Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 57Deutsches Elektronen-Synchrotron, 58Institut de Fisica d'Altes Energies, 59Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 60Max-Planck-Institut für Physik, München, Germany, 61Institut de Fisica d'Altes Energies, 62Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 63Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 64Max-Planck-Institut für Physik, München, Germany, 65Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 66ETH Zurich, Switzerland, 67Max-Planck-Institut für Physik, München, Germany, 68Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 69Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 70Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 71Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 72Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 73Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 74INAF National Institute for Astrophysics, Rome, Italy, 75Università di Udine, and INFN Trieste, Udine, Italy, 76Universidad Complutense, Madrid, Spain, 77Saha Institute of Nuclear Physics, Kolkata, India, 78Inst. for Nucl. Research and Nucl. Energy, Sofia, Bulgaria, 79Inst. for Nucl. Research and Nucl. Energy, Sofia, Bulgaria, 80Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 81Universität Würzburg, Würzburg, Germany, 82INAF National Institute for Astrophysics, Rome, Italy, 83Università di Padova and INFN, Padova, Italy, 84Institut de Fisica d'Altes Energies, 85Max-Planck-Institut für Physik, München, Germany, 86Max-Planck-Institut für Physik, München, Germany, 87Max-Planck-Institut für Physik, München, Germany, 88Institut de Fisica d'Altes Energies, 89Max-Planck-Institut für Physik, München, Germany, 90Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 91Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 92University of Łódź, Lodz, Poland, 93Universidad Complutense, Madrid, Spain, 94Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 95Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 96Max-Planck-Institut für Physik, München, Germany, 97Institut de Fisica d'Altes Energies, 98Università di Padova and INFN, Padova, Italy, 99Institut de Fisica d'Altes Energies, 100Università di Udine, and INFN Trieste, Udine, Italy, 101Max-Planck-Institut für Physik, München, Germany, 102Università di Siena, and INFN Pisa, Siena, Italy, 103Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 104Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 105Deutsches Elektronen-Synchrotron, 106Università di Udine, and INFN Trieste, Udine, Italy, 107INAF National Institute for Astrophysics, Rome, Italy, 108Università di Udine, and INFN Trieste, Udine, Italy, 109Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 110Università di Pisa, and INFN Pisa, Pisa, Italy, 111Università di Padova and INFN, Padova, Italy, 112Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 113Max-Planck-Institut für Physik, München, Germany, 114Università di Padova and INFN, Padova, Italy, 115Technische Universität Dortmund, Dortmund, Germany, 116Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 117Institut de Fisica d'Altes Energies, 118Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, Japan, 119Deutsches Elektronen-Synchrotron, 120Technische Universität Dortmund, Dortmund, Germany, 121Max-Planck-Institut für Physik, München, Germany, 122Università di Pisa, and INFN Pisa, Pisa, Italy, 123Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 124University of Łódź, Lodz, Poland, 125Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 126University of Łódź, Lodz, Poland, 127INAF National Institute for Astrophysics, Rome, Italy, 128Max-Planck-Institut für Physik, München, Germany, 129Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 130Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 131INAF National Institute for Astrophysics, Rome, Italy, 132Inst. for Nucl. Research and Nucl. Energy, Sofia, Bulgaria, 133Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 134Università di Padova and INFN, Padova, Italy, 135Max-Planck-Institut für Physik, München, Germany, 136ICREA and Institute for Space Sciences, 137Universitat de Barcelona, ICC, IEEC-UB, Barcelona, Spain, 138Max-Planck-Institut für Physik, München, Germany, 139Università di Udine, and INFN Trieste, Udine, Italy, 140Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 141Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 142Max-Planck-Institut für Physik, München, Germany, 143Institut de Fisica d'Altes Energies, 144Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 145Institute for Space Sciences, 146Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split - FESB, University of Zagreb - FER, University of Osijek, Croatia, 147Università di Udine, and INFN Trieste, Udine, Italy, 148Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 149Dip. di Fisica e Astronomia, Università di Bologna, Italy, 150KTH Royal Institute of Technology, Department of Physics, Stockholm, Sweden, 151INAF, Osservatorio Astrofisico di Torino, Pino Torinese, Italy, 152Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Finland, 153Aalto University Metsähovi Radio Observatory, Kylmälä, Finland, 154Aalto University Metsähovi Radio Observatory, Kylmälä, Finland, 155Aalto University Metsähovi Radio Observatory, Kylmälä, Finland, 156Aalto University Metsähovi Radio Observatory, Kylmälä, Finland, 157IAR, Boston University, USA, 158IAR, Boston University, USA, 159IAR, Boston University, USA, 160IAR, Boston University, USA, 161Physical Research Laboratory, Gujrat, India, 162Physical Research Laboratory, Gujrat, India, 163Physical Research Laboratory, Gujrat, India, 164Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 165Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 166Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 167Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 168Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 169Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 170Inst. de Astrofísica de Canarias, La Laguna, Tenerife, Spain, 171Department of Physics, Lancaster University, UK, 172Astrophysics Research Institute, Liverpool John Moores University, UK, 173St.Petersburg State University, Russia, 174Crimean Astrophysical Observatory, Crimea, 175St.Petersburg State University, Russia

Context. PKS 1510-089 is one of only a few flat spectrum radio quasars detected in the VHE (very-high-energy, > 100 GeV) gamma-ray band. Aims. Read More

2016Oct
Authors: IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, J. Auffenberg, S. Axani, X. Bai, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker-Tjus, K. -H. Becker, S. BenZvi, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, S. Blot, C. Bohm, M. Borner, F. Bos, D. Bose, S. Boser, O. Botner, J. Braun, L. Brayeur, H. -P. Bretz, S. Bron, A. Burgman, T. Carver, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen R. Cross, M. Day, J. P. A. M. de Andre, C. De Clercq, E. del Pino Rosendo, H. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, J. C. Diaz-Velez, V. di Lorenzo, H. Dujmovic, J. P. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, P. Eller, S. Euler, P. A. Evenson, S. Fahey, A. R. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C. -C. Fosig, A. Franckowiak, R. Franke, E. Friedman, T. Fuchs, T. K. Gaisser, J. Gallagher, L. Gerhardt, K. Ghorbani, W. Giang, L. Gladstone, T. Glauch, T. Glusenkamp, A. Goldschmidt, G. Golup, J. G. Gonzalez, D. Grant, Z. Griffith, C. Haack, A. Haj Ismail, A. Hallgren, F. Halzen, E. Hansen, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, K. Holzapfel, K. Hoshina, F. Huang, M. Huber, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, M. Jurkovic, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, A. Kheirandish, M. Kim, T. Kintscher, J. Kiryluk, T. Kittler, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Kopke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, M. Kroll, G. Kruckl, C. Kruger, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, M. J. Larson, F. Lauber, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, L. Lu, J. Lunemann, J. Madsen, G. Maggi, K. B. M. Mahn, S. Mancina, M. Mandelartz, R. Maruyama, K. Mase, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, L. Mohrmann, T. Montaruli, M. Moulai, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. O'Murchadha, T. Palczewski, H. Pandya, D. V. Pankova, P. Peiffer, O. Penek, J. A. Pepper, C. Perez de los Heros, D. Pieloth, E. Pinat, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Radel, M. Rameez, K. Rawlins, R. Reimann, B. Relethford, M. Relich, E. Resconi, W. Rhode, M. Richman, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, L. Sabbatini, S. E. Sanchez-Herrera, A. Sandrock, J. Sandroos, S. Sarkar, K. Satalecka, P. Schlunder, T. Schmidt, S. Schoenen, S. Schoneberg, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, T. Stanev, A. Stasik, J. Stettner, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stossl, R. Strom, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, F. Tenholt, S. Ter-Antonyan, A. Terliuk, G. Tevsic, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, M. van Rossem, J. van Santen, J. Veenkamp, M. Vehring, M. Voge, E. Vogel, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, Ch. Weaver, M. J. Weiss, C. Wendt, S. Westerhoff, B. J. Whelan, S. Wickmann, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, M. Wolf, T. R. Wood, E. Woolsey, K. Woschnagg, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, M. Zoll MAGIC Collaboration, :, M. L. Ahnen, S. Ansoldi, L. A. Antonelli, P. Antoranz, A. Babic, B. Banerjee, P. Bangale, U. Barres de Almeida, J. A. Barrio, J. Becerra Gonzalez, W. Bednarek, E. Bernardini, A. Berti, B. Biasuzzi, A. Biland, O. Blanch, S. Bonnefoy, G. Bonnoli, F. Borracci, T. Bretz, S. Buson, A. Carosi, A. Chatterjee, R. Clavero, P. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, E. de Ona Wilhelmi, F. Di Pierro, M. Doert, A. Dominguez, D. Dominis Prester, D. Dorner, M. Doro, S. Einecke, D. Eisenacher Glawion, D. Elsaesser, M. Engelkemeier, V. Fallah Ramazani, A. Fernandez-Barral, D. Fidalgo, M. V. Fonseca, L. Font, K. Frantzen, C. Fruck, D. Galindo, R. J. Garcia Lopez, M. Garczarczyk, D. Garrido Terrats, M. Gaug, P. Giammaria, N. Godinovic, A. Gonzalez Munoz, D. Gora, D. Guberman, D. Hadasch, A. Hahn, Y. Hanabata, M. Hayashida, J. Herrera, J. Hose, D. Hrupec, G. Hughes, W. Idec, K. Kodani, Y. Konno, H. Kubo, J. Kushida, A. La Barbera, D. Lelas, E. Lindfors, S. Lombardi, F. Longo, M. Lopez, R. Lopez-Coto, P. Majumdar, M. Makariev, K. Mallot, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, B. Marcote, M. Mariotti, M. Martinez, D. Mazin, U. Menzel, J. M. Miranda, R. Mirzoyan, A. Moralejo, E. Moretti, D. Nakajima, V. Neustroev, A. Niedzwiecki, M. Nievas Rosillo, K. Nilsson, K. Nishijima, K. Noda, L. Nogues, A. Overkemping, S. Paiano, J. Palacio, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, X. Paredes-Fortuny, G. Pedaletti, M. Peresano, L. Perri, M. Persic, J. Poutanen, P. G. Prada Moroni, E. Prandini, I. Puljak, I. Reichardt, W. Rhode, M. Ribo, J. Rico, J. Rodriguez Garcia, T. Saito, K. Satalecka, S. Schroeder, C. Schultz, T. Schweizer, A. Sillanpaa, J. Sitarek, I. Snidaric, D. Sobczynska, A. Stamerra, T. Steinbring, M. Strzys, T. Suric, L. Takalo, F. Tavecchio, P. Temnikov, T. Terzic, D. Tescaro, M. Teshima, J. Thaele, D. F. Torres, T. Toyama, A. Treves, G. Vanzo, V. Verguilov, I. Vovk, J. E. Ward, M. Will, M. H. Wu, R. Zanin VERITAS Collaboration, :, A. U. Abeysekara, S. Archambault, A. Archer, W. Benbow, R. Bird, E. Bourbeau, M. Buchovecky, V. Bugaev, K. Byrum, J. V Cardenzana, M. Cerruti, L. Ciupik, M. P. Connolly, W. Cui, H. J. Dickinson, J. Dumm, J. D. Eisch, M. Errando, A. Falcone, Q. Feng, J. P. Finley, H. Fleischhack, A. Flinders, L. Fortson, A. Furniss, G. H. Gillanders, S. Griffin, J. Grube, M. Hutten, N. Haakansson, O. Hervet, J. Holder, T. B. Humensky, C. A. Johnson, P. Kaaret, P. Kar, N. Kelley-Hoskins, M. Kertzman, D. Kieda, M. Krause, F. Krennrich, S. Kumar, M. J. Lang, G. Maier, S. McArthur, A. McCann, P. Moriarty, R. Mukherjee, T. Nguyen, D. Nieto, S. O'Brien, R. A. Ong, A. N. Otte, N. Park, M. Pohl, A. Popkow, E. Pueschel, J. Quinn, K. Ragan, P. T. Reynolds, G. T. Richards, E. Roache, C. Rulten, I. Sadeh, M. Santander, G. H. Sembroski, K. Shahinyan, D. Staszak, I. Telezhinsky, J. V. Tucci, J. Tyler, S. P. Wakely, A. Weinstein, P. Wilcox, A. Wilhelm, D. A. Williams, B. Zitzer

We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescopes (MAGIC and VERITAS). While IceCube is capable of monitoring the whole sky continuously, high-energy gamma-ray telescopes have restricted fields of view and in general are unlikely to be observing a potential neutrino-flaring source at the time such neutrinos are recorded. The use of neutrino-triggered alerts thus aims at increasing the availability of simultaneous multi-messenger data during potential neutrino flaring activity, which can increase the discovery potential and constrain the phenomenological interpretation of the high-energy emission of selected source classes (e. Read More

The measurement of the direction of WIMP-induced nuclear recoils is a compelling but technologically challenging strategy to provide an unambiguous signature of the detection of Galactic dark matter. Most directional detectors aim to reconstruct the dark-matter-induced nuclear recoil tracks, either in gas or solid targets. The main challenge with directional detection is the need for high spatial resolution over large volumes, which puts strong requirements on the readout technologies. Read More

2016Sep
Affiliations: 1SRL/Caltech, 2SSL/UC Berkeley, 3STEL Nagoya University, 4Remeis-Observatory & ECAP, 5U Michigan, 6SSL/UC Berkeley, 7Laboratoire AIM, CEA/IRFU, 8IoA Cambridge, 9CfA Harvard, 10SRL/Caltech, 11Laboratoire AIM, CEA/IRFU, 12U Iowa, 13Sabanci U, 14ESAC, 15International Centre for Radio Astronomy Research - Curtin U, 16CRESST/UMBC, 17ESO, 18Laboratoire AIM, CEA/IRFU, 19JPL, 20ESAC, 21JPL, 22Remeis-Observatory & ECAP

We present a detailed spectral analysis of XMM-Newton and NuSTAR observations of the accreting transient black hole GRS 1739-278 during a very faint low hard state at ~0.02% of the Eddington luminosity (for a distance of 8.5 kpc and a mass of 10 M_sun ). Read More

The most compelling candidates for Dark Matter to day are WIMPs and axions. The applicability of gasesous Time Projection Chambers (TPCs) with Micromesh Gas Structures (Micromegas) to the search of these particles is explored within this work. Both particles would produce an extremely low rate at very low energies in particle detectors. Read More

This paper addresses channel estimation and data equalization on frequency-selective 1-bit quantized Multiple Input-Multiple Output (MIMO) systems. No joint processing or Channel State Information is assumed at the transmitter, and therefore our findings are also applicable to the uplink of Multi-User MIMO systems. System models for both Orthogonal Division Frequency Multiplexing (OFDM) and single-carrier schemes are developed. Read More

The valence and spin state evolution of Mn and Co on TbMn$_{\rm 1-x}$Co$_{\rm x}$O$_3$ series is precisely determined by means of soft and hard x-ray absorption spectroscopy (XAS) and K$\beta$ x-ray emission spectroscopy (XES). Our results show the change from Mn$^{3+}$ to Mn$^{4+}$ both high-spin (HS) together with the evolution from Co$^{2+}$ HS to Co$^{3+}$ low-spin (LS) with increasing $\rm x$. In addition, high energy resolution XAS spectra on the K pre-edge region are interpreted in terms of the strong charge transfer and hybridization effects along the series. Read More

We analyze 15,000 spectra of 29 stellar-mass black hole candidates collected over the 16-year mission lifetime of RXTE using a simple phenomenological model. As these black holes vary widely in luminosity and progress through a sequence of spectral states, which we broadly refer to as hard and soft, we focus on two spectral components: The Compton power law and the reflection spectrum it generates by illuminating the accretion disk. Our proxy for the strength of reflection is the equivalent width of the Fe-K line as measured with respect to the power law. Read More

2016Sep
Authors: MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, P. Antoranz4, C. Arcaro5, A. Babic6, B. Banerjee7, P. Bangale8, U. Barres de Almeida9, J. A. Barrio10, J. Becerra González11, W. Bednarek12, E. Bernardini13, A. Berti14, B. Biasuzzi15, A. Biland16, O. Blanch17, S. Bonnefoy18, G. Bonnoli19, F. Borracci20, T. Bretz21, S. Buson22, A. Carosi23, A. Chatterjee24, R. Clavero25, P. Colin26, E. Colombo27, J. L. Contreras28, J. Cortina29, S. Covino30, P. Da Vela31, F. Dazzi32, A. De Angelis33, B. De Lotto34, E. de Oña Wilhelmi35, F. Di Pierro36, M. Doert37, A. Domínguez38, D. Dominis Prester39, D. Dorner40, M. Doro41, S. Einecke42, D. Eisenacher Glawion43, D. Elsaesser44, M. Engelkemeier45, V. Fallah Ramazani46, A. Fernández-Barral47, D. Fidalgo48, M. V. Fonseca49, L. Font50, K. Frantzen51, C. Fruck52, D. Galindo53, R. J. García López54, M. Garczarczyk55, D. Garrido Terrats56, M. Gaug57, P. Giammaria58, N. Godinović59, D. Gora60, D. Guberman61, D. Hadasch62, A. Hahn63, M. Hayashida64, J. Herrera65, J. Hose66, D. Hrupec67, G. Hughes68, W. Idec69, K. Kodani70, Y. Konno71, H. Kubo72, J. Kushida73, A. La Barbera74, D. Lelas75, E. Lindfors76, S. Lombardi77, F. Longo78, M. López79, R. López-Coto80, P. Majumdar81, M. Makariev82, K. Mallot83, G. Maneva84, M. Manganaro85, K. Mannheim86, L. Maraschi87, B. Marcote88, M. Mariotti89, M. Martínez90, D. Mazin91, U. Menzel92, J. M. Miranda93, R. Mirzoyan94, A. Moralejo95, E. Moretti96, D. Nakajima97, V. Neustroev98, A. Niedzwiecki99, M. Nievas Rosillo100, K. Nilsson101, K. Nishijima102, K. Noda103, L. Nogués104, S. Paiano105, J. Palacio106, M. Palatiello107, D. Paneque108, R. Paoletti109, J. M. Paredes110, X. Paredes-Fortuny111, G. Pedaletti112, M. Peresano113, L. Perri114, M. Persic115, J. Poutanen116, P. G. Prada Moroni117, E. Prandini118, I. Puljak119, J. R. Garcia120, I. Reichardt121, W. Rhode122, M. Ribó123, J. Rico124, T. Saito125, K. Satalecka126, S. Schroeder127, T. Schweizer128, S. N. Shore129, A. Sillanpää130, J. Sitarek131, I. Snidaric132, D. Sobczynska133, A. Stamerra134, M. Strzys135, T. Surić136, L. Takalo137, F. Tavecchio138, P. Temnikov139, T. Terzić140, D. Tescaro141, M. Teshima142, D. F. Torres143, T. Toyama144, A. Treves145, G. Vanzo146, V. Verguilov147, I. Vovk148, J. E. Ward149, M. Will150, M. H. Wu151, R. Zanin152, R. Desiante153
Affiliations: 1ETH Zurich, CH-8093 Zurich, Switzerland, 2Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 3INAF National Institute for Astrophysics, I-00136 Rome, Italy, 4Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 5Università di Padova and INFN, I-35131 Padova, Italy, 6Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 7Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 8Max-Planck-Institut für Physik, D-80805 München, Germany, 9Max-Planck-Institut für Physik, D-80805 München, Germany, 10Universidad Complutense, E-28040 Madrid, Spain, 11Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 12University of Łódź, PL-90236 Lodz, Poland, 13Deutsches Elektronen-Synchrotron, 14Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 15Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 16ETH Zurich, CH-8093 Zurich, Switzerland, 17Institut de Fisica d'Altes Energies, 18Universidad Complutense, E-28040 Madrid, Spain, 19Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 20Max-Planck-Institut für Physik, D-80805 München, Germany, 21Universität Würzburg, D-97074 Würzburg, Germany, 22Università di Padova and INFN, I-35131 Padova, Italy, 23INAF National Institute for Astrophysics, I-00136 Rome, Italy, 24Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 25Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 26Max-Planck-Institut für Physik, D-80805 München, Germany, 27Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 28Universidad Complutense, E-28040 Madrid, Spain, 29Institut de Fisica d'Altes Energies, 30INAF National Institute for Astrophysics, I-00136 Rome, Italy, 31Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 32Max-Planck-Institut für Physik, D-80805 München, Germany, 33Università di Padova and INFN, I-35131 Padova, Italy, 34Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 35Institute for Space Sciences, 36INAF National Institute for Astrophysics, I-00136 Rome, Italy, 37Technische Universität Dortmund, D-44221 Dortmund, Germany, 38Universidad Complutense, E-28040 Madrid, Spain, 39Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 40Universität Würzburg, D-97074 Würzburg, Germany, 41Università di Padova and INFN, I-35131 Padova, Italy, 42Technische Universität Dortmund, D-44221 Dortmund, Germany, 43Universität Würzburg, D-97074 Würzburg, Germany, 44Technische Universität Dortmund, D-44221 Dortmund, Germany, 45Technische Universität Dortmund, D-44221 Dortmund, Germany, 46Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 47Institut de Fisica d'Altes Energies, 48Universidad Complutense, E-28040 Madrid, Spain, 49Universidad Complutense, E-28040 Madrid, Spain, 50Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 51Technische Universität Dortmund, D-44221 Dortmund, Germany, 52Max-Planck-Institut für Physik, D-80805 München, Germany, 53Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 54Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 55Deutsches Elektronen-Synchrotron, 56Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 57Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 58INAF National Institute for Astrophysics, I-00136 Rome, Italy, 59Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 60Deutsches Elektronen-Synchrotron, 61Institut de Fisica d'Altes Energies, 62Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 63Max-Planck-Institut für Physik, D-80805 München, Germany, 64Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 65Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 66Max-Planck-Institut für Physik, D-80805 München, Germany, 67Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 68ETH Zurich, CH-8093 Zurich, Switzerland, 69University of Łódź, PL-90236 Lodz, Poland, 70Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 71Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 72Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 73Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 74INAF National Institute for Astrophysics, I-00136 Rome, Italy, 75Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 76Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 77INAF National Institute for Astrophysics, I-00136 Rome, Italy, 78Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 79Universidad Complutense, E-28040 Madrid, Spain, 80Institut de Fisica d'Altes Energies, 81Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 82Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 83Deutsches Elektronen-Synchrotron, 84Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 85Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 86Universität Würzburg, D-97074 Würzburg, Germany, 87INAF National Institute for Astrophysics, I-00136 Rome, Italy, 88Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 89Università di Padova and INFN, I-35131 Padova, Italy, 90Institut de Fisica d'Altes Energies, 91Max-Planck-Institut für Physik, D-80805 München, Germany, 92Max-Planck-Institut für Physik, D-80805 München, Germany, 93Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 94Max-Planck-Institut für Physik, D-80805 München, Germany, 95Institut de Fisica d'Altes Energies, 96Max-Planck-Institut für Physik, D-80805 München, Germany, 97Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 98Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 99University of Łódź, PL-90236 Lodz, Poland, 100Universidad Complutense, E-28040 Madrid, Spain, 101Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 102Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 103Max-Planck-Institut für Physik, D-80805 München, Germany, 104Institut de Fisica d'Altes Energies, 105Università di Padova and INFN, I-35131 Padova, Italy, 106Institut de Fisica d'Altes Energies, 107Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 108Max-Planck-Institut für Physik, D-80805 München, Germany, 109Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 110Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 111Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 112Deutsches Elektronen-Synchrotron, 113Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 114INAF National Institute for Astrophysics, I-00136 Rome, Italy, 115Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 116Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 117Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy, 118ETH Zurich, CH-8093 Zurich, Switzerland, 119Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 120Max-Planck-Institut für Physik, D-80805 München, Germany, 121Università di Padova and INFN, I-35131 Padova, Italy, 122Technische Universität Dortmund, D-44221 Dortmund, Germany, 123Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 124Institut de Fisica d'Altes Energies, 125Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 126Deutsches Elektronen-Synchrotron, 127Technische Universität Dortmund, D-44221 Dortmund, Germany, 128Max-Planck-Institut für Physik, D-80805 München, Germany, 129Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy, 130Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 131University of Łódź, PL-90236 Lodz, Poland, 132Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 133University of Łódź, PL-90236 Lodz, Poland, 134INAF National Institute for Astrophysics, I-00136 Rome, Italy, 135Max-Planck-Institut für Physik, D-80805 München, Germany, 136Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 137Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 138INAF National Institute for Astrophysics, I-00136 Rome, Italy, 139Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 140Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 141Università di Padova and INFN, I-35131 Padova, Italy, 142Max-Planck-Institut für Physik, D-80805 München, Germany, 143ICREA and Institute for Space Sciences, 144Max-Planck-Institut für Physik, D-80805 München, Germany, 145Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 146Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 147Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 148Max-Planck-Institut für Physik, D-80805 München, Germany, 149Institut de Fisica d'Altes Energies, 150Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 151Institute for Space Sciences, 152Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 153Università di Udine, and INFN Trieste, I-33100 Udine, Italy

Context. QSO B0218+357 is a gravitationally lensed blazar located at a redshift of 0.944. Read More

We demonstrate an optical fiber fault location method based on the frequency response of the modulated fiber optical backscattered signal in a steady state low-frequency step regime. Careful calibration and measurement allows for the reconstruction of the fiber transfer function, which, associated to its mathematical model, is capable of extracting the fiber characteristics. The technique is capable of identifying non-reflective fault events in an optical fiber link and is perfectly compatible with previous methods that focus on the reflective events. Read More

We present first results from a series of $NuSTAR$ observations of the black hole X-ray binary V404 Cyg obtained during its summer 2015 outburst, primarily focusing on observations during the height of this outburst activity. The $NuSTAR$ data show extreme variability in both the flux and spectral properties of the source. This is partly driven by strong and variable line-of-sight absorption, similar to previous outbursts. Read More

2016Aug
Authors: The CLIC, CLICdp collaborations, :, M. J. Boland, U. Felzmann, P. J. Giansiracusa, T. G. Lucas, R. P. Rassool, C. Balazs, T. K. Charles, K. Afanaciev, I. Emeliantchik, A. Ignatenko, V. Makarenko, N. Shumeiko, A. Patapenka, I. Zhuk, A. C. Abusleme Hoffman, M. A. Diaz Gutierrez, M. Vogel Gonzalez, Y. Chi, X. He, G. Pei, S. Pei, G. Shu, X. Wang, J. Zhang, F. Zhao, Z. Zhou, H. Chen, Y. Gao, W. Huang, Y. P. Kuang, B. Li, Y. Li, J. Shao, J. Shi, C. Tang, X. Wu, L. Ma, Y. Han, W. Fang, Q. Gu, D. Huang, X. Huang, J. Tan, Z. Wang, Z. Zhao, T. Laštovička, U. Uggerhoj, T. N. Wistisen, A. Aabloo, K. Eimre, K. Kuppart, S. Vigonski, V. Zadin, M. Aicheler, E. Baibuz, E. Brücken, F. Djurabekova, P. Eerola, F. Garcia, E. Haeggström, K. Huitu, V. Jansson, V. Karimaki, I. Kassamakov, A. Kyritsakis, S. Lehti, A. Meriläinen, R. Montonen, T. Niinikoski, K. Nordlund, K. Österberg, M. Parekh, N. A. Törnqvist, J. Väinölä, M. Veske, W. Farabolini, A. Mollard, O. Napoly, F. Peauger, J. Plouin, P. Bambade, I. Chaikovska, R. Chehab, M. Davier, W. Kaabi, E. Kou, F. LeDiberder, R. Pöschl, D. Zerwas, B. Aimard, G. Balik, J. -P. Baud, J. -J. Blaising, L. Brunetti, M. Chefdeville, C. Drancourt, N. Geoffroy, J. Jacquemier, A. Jeremie, Y. Karyotakis, J. M. Nappa, S. Vilalte, G. Vouters, A. Bernard, I. Peric, M. Gabriel, F. Simon, M. Szalay, N. van der Kolk, T. Alexopoulos, E. N. Gazis, N. Gazis, E. Ikarios, V. Kostopoulos, S. Kourkoulis, P. D. Gupta, P. Shrivastava, H. Arfaei, M. K. Dayyani, H. Ghasem, S. S. Hajari, H. Shaker, Y. Ashkenazy, H. Abramowicz, Y. Benhammou, O. Borysov, S. Kananov, A. Levy, I. Levy, O. Rosenblat, G. D'Auria, S. Di Mitri, T. Abe, A. Aryshev, T. Higo, Y. Makida, S. Matsumoto, T. Shidara, T. Takatomi, Y. Takubo, T. Tauchi, N. Toge, K. Ueno, J. Urakawa, A. Yamamoto, M. Yamanaka, R. Raboanary, R. Hart, H. van der Graaf, G. Eigen, J. Zalieckas, E. Adli, R. Lillestøl, L. Malina, J. Pfingstner, K. N. Sjobak, W. Ahmed, M. I. Asghar, H. Hoorani, S. Bugiel, R. Dasgupta, M. Firlej, T. A. Fiutowski, M. Idzik, M. Kopec, M. Kuczynska, J. Moron, K. P. Swientek, W. Daniluk, B. Krupa, M. Kucharczyk, T. Lesiak, A. Moszczynski, B. Pawlik, P. Sopicki, T. Wojtoń, L. Zawiejski, J. Kalinowski, M. Krawczyk, A. F. Żarnecki, E. Firu, V. Ghenescu, A. T. Neagu, T. Preda, I-S. Zgura, A. Aloev, N. Azaryan, J. Budagov, M. Chizhov, M. Filippova, V. Glagolev, A. Gongadze, S. Grigoryan, D. Gudkov, V. Karjavine, M. Lyablin, A. Olyunin, A. Samochkine, A. Sapronov, G. Shirkov, V. Soldatov, A. Solodko, E. Solodko, G. Trubnikov, I. Tyapkin, V. Uzhinsky, A. Vorozhtov, E. Levichev, N. Mezentsev, P. Piminov, D. Shatilov, P. Vobly, K. Zolotarev, I. Bozovic Jelisavcic, G. Kacarevic, S. Lukic, G. Milutinovic-Dumbelovic, M. Pandurovic, U. Iriso, F. Perez, M. Pont, J. Trenado, M. Aguilar-Benitez, J. Calero, L. Garcia-Tabares, D. Gavela, J. L. Gutierrez, D. Lopez, F. Toral, D. Moya, A. Ruiz Jimeno, I. Vila, T. Argyropoulos, C. Blanch Gutierrez, M. Boronat, D. Esperante, A. Faus-Golfe, J. Fuster, N. Fuster Martinez, N. Galindo Muñoz, I. García, J. Giner Navarro, E. Ros, M. Vos, R. Brenner, T. Ekelöf, M. Jacewicz, J. Ögren, M. Olvegård, R. Ruber, V. Ziemann, D. Aguglia, N. Alipour Tehrani, A. Andersson, F. Andrianala, F. Antoniou, K. Artoos, S. Atieh, R. Ballabriga Sune, M. J. Barnes, J. Barranco Garcia, H. Bartosik, C. Belver-Aguilar, A. Benot Morell, D. R. Bett, S. Bettoni, G. Blanchot, O. Blanco Garcia, X. A. Bonnin, O. Brunner, H. Burkhardt, S. Calatroni, M. Campbell, N. Catalan Lasheras, M. Cerqueira Bastos, A. Cherif, E. Chevallay, B. Constance, R. Corsini, B. Cure, S. Curt, B. Dalena, D. Dannheim, G. De Michele, L. De Oliveira, N. Deelen, J. P. Delahaye, T. Dobers, S. Doebert, M. Draper, F. Duarte Ramos, A. Dubrovskiy, K. Elsener, J. Esberg, M. Esposito, V. Fedosseev, P. Ferracin, A. Fiergolski, K. Foraz, A. Fowler, F. Friebel, J-F. Fuchs, C. A. Fuentes Rojas, A. Gaddi, L. Garcia Fajardo, H. Garcia Morales, C. Garion, L. Gatignon, J-C. Gayde, H. Gerwig, A. N. Goldblatt, C. Grefe, A. Grudiev, F. G. Guillot-Vignot, M. L. Gutt-Mostowy, M. Hauschild, C. Hessler, J. K. Holma, E. Holzer, M. Hourican, D. Hynds, Y. Inntjore Levinsen, B. Jeanneret, E. Jensen, M. Jonker, M. Kastriotou, J. M. K. Kemppinen, R. B. Kieffer, W. Klempt, O. Kononenko, A. Korsback, E. Koukovini Platia, J. W. Kovermann, C-I. Kozsar, I. Kremastiotis, S. Kulis, A. Latina, F. Leaux, P. Lebrun, T. Lefevre, L. Linssen, X. Llopart Cudie, A. A. Maier, H. Mainaud Durand, E. Manosperti, C. Marelli, E. Marin Lacoma, R. Martin, S. Mazzoni, G. Mcmonagle, O. Mete, L. M. Mether, M. Modena, R. M. Münker, T. Muranaka, E. Nebot Del Busto, N. Nikiforou, D. Nisbet, J-M. Nonglaton, F. X. Nuiry, A. Nürnberg, M. Olvegard, J. Osborne, S. Papadopoulou, Y. Papaphilippou, A. Passarelli, M. Patecki, L. Pazdera, D. Pellegrini, K. Pepitone, E. Perez Codina, A. Perez Fontenla, T. H. B. Persson, M. Petrič, F. Pitters, S. Pittet, F. Plassard, R. Rajamak, S. Redford, Y. Renier, S. F. Rey, G. Riddone, L. Rinolfi, E. Rodriguez Castro, P. Roloff, C. Rossi, V. Rude, G. Rumolo, A. Sailer, E. Santin, D. Schlatter, H. Schmickler, D. Schulte, N. Shipman, E. Sicking, R. Simoniello, P. K. Skowronski, P. Sobrino Mompean, L. Soby, M. P. Sosin, S. Sroka, S. Stapnes, G. Sterbini, R. Ström, I. Syratchev, F. Tecker, P. A. Thonet, L. Timeo, H. Timko, R. Tomas Garcia, P. Valerio, A. L. Vamvakas, A. Vivoli, M. A. Weber, R. Wegner, M. Wendt, B. Woolley, W. Wuensch, J. Uythoven, H. Zha, P. Zisopoulos, M. Benoit, M. Vicente Barreto Pinto, M. Bopp, H. H. Braun, M. Csatari Divall, M. Dehler, T. Garvey, J. Y. Raguin, L. Rivkin, R. Zennaro, A. Aksoy, Z. Nergiz, E. Pilicer, I. Tapan, O. Yavas, V. Baturin, R. Kholodov, S. Lebedynskyi, V. Miroshnichenko, S. Mordyk, I. Profatilova, V. Storizhko, N. Watson, A. Winter, J. Goldstein, S. Green, J. S. Marshall, M. A. Thomson, B. Xu, W. A. Gillespie, R. Pan, M. A Tyrk, D. Protopopescu, A. Robson, R. Apsimon, I. Bailey, G. Burt, D. Constable, A. Dexter, S. Karimian, C. Lingwood, M. D. Buckland, G. Casse, J. Vossebeld, A. Bosco, P. Karataev, K. Kruchinin, K. Lekomtsev, L. Nevay, J. Snuverink, E. Yamakawa, V. Boisvert, S. Boogert, G. Boorman, S. Gibson, A. Lyapin, W. Shields, P. Teixeira-Dias, S. West, R. Jones, N. Joshi, R. Bodenstein, P. N. Burrows, G. B. Christian, D. Gamba, C. Perry, J. Roberts, J. A. Clarke, N. A. Collomb, S. P. Jamison, B. J. A. Shepherd, D. Walsh, M. Demarteau, J. Repond, H. Weerts, L. Xia, J. D. Wells, C. Adolphsen, T. Barklow, M. Breidenbach, N. Graf, J. Hewett, T. Markiewicz, D. McCormick, K. Moffeit, Y. Nosochkov, M. Oriunno, N. Phinney, T. Rizzo, S. Tantawi, F. Wang, J. Wang, G. White, M. Woodley

The Compact Linear Collider (CLIC) is a multi-TeV high-luminosity linear e+e- collider under development. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in a staged approach with three centre-of-mass energy stages ranging from a few hundred GeV up to 3 TeV. The first stage will focus on precision Standard Model physics, in particular Higgs and top-quark measurements. Read More

LOFT-P is a concept for a NASA Astrophysics Probe-Class (<$1B) X-ray timing mission, based on the LOFT concept originally proposed to ESAs M3 and M4 calls. LOFT-P requires very large collecting area (>6 m^2, >10x RXTE), high time resolution, good spectral resolution, broad-band spectral coverage (2-30 keV), highly flexible scheduling, and an ability to detect and respond promptly to time-critical targets of opportunity. It addresses science questions such as: What is the equation of state of ultra dense matter? What are the effects of strong gravity on matter spiraling into black holes? It would be optimized for sub-millisecond timing to study phenomena at the natural timescales of neutron star surfaces and black hole event horizons and to measure mass and spin of black holes. Read More

We report on the performance of the statistical, X-ray absorption lines identification procedure XLINE-ID. As illustration, it is used to estimate the time averaged gas density $n_H(r)$ of a representative AGN's warm absorber ($T\approx 10^5$~K) X-ray simulated spectrum. The method relies on three key ingredients: (1) a well established emission continuum level; (2) a robust grid of photoionisation models spanning several orders of magnitude in gas density ($n_H$), plasma column density ($N_H$), and in ionization states; (3) theoretical curves of growth for a large set of atomic lines. Read More

In the context of AdS/CFT we provide analytical support for the proposed duality between a Wilson loop with a cusp, the cusp anomalous dimension, and the meson model constructed from a rotating open string with high angular momentum. This duality was previously studied using numerical tools in [1]. Our result implies that the minimum of the profile function of the minimal area surface dual to the Wilson loop, is related to the inverse of the bulk penetration of the dual string that hangs from the quark--anti-quark pair (meson) in the gauge theory. Read More

We present the first X-ray reflection model for testing the assumption that the metric of astrophysical black holes is described by the Kerr solution. We employ the formalism of the transfer function proposed by Cunningham. The calculations of the reflection spectrum of a thin accretion disk are split into two parts: the calculation of the transfer function and the calculation of the local spectrum at any emission point in the disk. Read More

The morphologies of crystalline lithium peroxide (Li2O2) discharge products in Li-O2 batteries have been shown to exhibit a dependency on subtle variations within the battery cell-operating environment including exposure to ambient air, moisture, or additives. As a result, imaging battery discharge products in real time under carefully controlled environmental conditions is a challenging obstacle for complete mechanistic understanding of Li2O2 growth and deposition during discharge in metal-air batteries. Here, we report the design of a completely enclosed cell for high-resolution in situ AFM imaging of Li-O2 battery discharge products. Read More

Conventional neuroimaging analyses have revealed the computational specificity of localized brain regions, exploiting the power of the subtraction technique in fMRI and event-related potential analyses in EEG. Moving beyond this convention, many researchers have begun exploring network-based neurodynamics and coordination between brain regions as a function of behavioral parameters or environmental statistics; however, most approaches average evoked activity across the experimental session to study task-dependent networks. Here, we examined on-going oscillatory activity and use a methodology to estimate directionality in brain-behavior interactions. Read More

We present a study of the detectability of CO molecules in the Galactic interstellar medium using high-resolution X-ray spectra obtained with the XMM-Newton Reflection Grating Spectrometer. We analyzed 10 bright low mass X-ray binaries (LMXBs) to study the CO contribution in their line-of-sights. A total of 25 observations were fitted with the ISMabs X-ray absorption model which includes photoabsorption cross-sections for O I, O II, O III and CO. Read More

The efficient production of electricity from nuclear fusion in magnetically confined plasmas relies on a good confinement of the thermal energy. For more than thirty years, the observation that such confinement depends on the mass of the plasma isotope and its interaction with apparently unrelated plasma conditions has remained largely unexplained and it has become one of the main unsolved issues. By means of numerical studies based on the gyrokinetic theory, we quantitatively show how the plasma microturbulence depends on the isotope mass through nonlinear multiscale microturbulence effects involving the interplay between zonal flows, electromagnetic effects and the torque applied. Read More

2016May
Authors: MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, P. Antoranz4, A. Babic5, B. Banerjee6, P. Bangale7, U. Barres de Almeida8, J. A. Barrio9, J. Becerra González10, W. Bednarek11, E. Bernardini12, B. Biasuzzi13, A. Biland14, O. Blanch15, S. Bonnefoy16, G. Bonnoli17, F. Borracci18, T. Bretz19, S. Buson20, A. Carosi21, A. Chatterjee22, R. Clavero23, P. Colin24, E. Colombo25, J. L. Contreras26, J. Cortina27, S. Covino28, P. Da Vela29, F. Dazzi30, A. De Angelis31, B. De Lotto32, E. de Oña Wilhelmi33, F. Di Pierro34, A. Domínguez35, D. Dominis Prester36, D. Dorner37, M. Doro38, S. Einecke39, D. Eisenacher Glawion40, D. Elsaesser41, A. Fernández-Barral42, D. Fidalgo43, M. V. Fonseca44, L. Font45, K. Frantzen46, C. Fruck47, D. Galindo48, R. J. García López49, M. Garczarczyk50, D. Garrido Terrats51, M. Gaug52, P. Giammaria53, N. Godinović54, A. González Muñoz55, D. Gora56, D. Guberman57, D. Hadasch58, A. Hahn59, Y. Hanabata60, M. Hayashida61, J. Herrera62, J. Hose63, D. Hrupec64, G. Hughes65, W. Idec66, K. Kodani67, Y. Konno68, H. Kubo69, J. Kushida70, A. La Barbera71, D. Lelas72, E. Lindfors73, S. Lombardi74, F. Longo75, M. López76, R. López-Coto77, P. Majumdar78, M. Makariev79, K. Mallot80, G. Maneva81, M. Manganaro82, K. Mannheim83, L. Maraschi84, B. Marcote85, M. Mariotti86, M. Martínez87, D. Mazin88, U. Menzel89, J. M. Miranda90, R. Mirzoyan91, A. Moralejo92, E. Moretti93, D. Nakajima94, V. Neustroev95, A. Niedzwiecki96, M. Nievas Rosillo97, K. Nilsson98, K. Nishijima99, K. Noda100, L. Nogués101, R. Orito102, A. Overkemping103, S. Paiano104, J. Palacio105, M. Palatiello106, D. Paneque107, R. Paoletti108, J. M. Paredes109, X. Paredes-Fortuny110, G. Pedaletti111, L. Perri112, M. Persic113, J. Poutanen114, P. G. Prada Moroni115, E. Prandini116, I. Puljak117, W. Rhode118, M. Ribó119, J. Rico120, J. Rodriguez Garcia121, T. Saito122, K. Satalecka123, C. Schultz124, T. Schweizer125, S. N. Shore126, A. Sillanpää127, J. Sitarek128, I. Snidaric129, D. Sobczynska130, A. Stamerra131, T. Steinbring132, M. Strzys133, L. Takalo134, H. Takami135, F. Tavecchio136, P. Temnikov137, T. Terzić138, D. Tescaro139, M. Teshima140, J. Thaele141, D. F. Torres142, T. Toyama143, A. Treves144, V. Verguilov145, I. Vovk146, J. E. Ward147, M. Will148, M. H. Wu149, R. Zanin150, D. A. Blinov151, W. P. Chen152, N. V. Efimova153, E. Forné154, T. S. Grishina155, T. Hovatta156, B. Jordan157, G. N. Kimeridze158, E. N. Kopatskaya159, E. Koptelova160, O. M. Kurtanidze161, S. O. Kurtanidze162, A. Lähteenmaäki163, V. M. Larionov164, E. G. Larionova165, L. V. Larionova166, R. Ligustri167, H. C. Lin168, B. McBreen169, D. A. Morozova170, M. G. Nikolashvili171, C. M. Raiteri172, J. A. Ros173, A. C. Sadun174, L. A. Sigua175, M. Tornikoski176, I. S. Troitsky177, M. Villata178
Affiliations: 1ETH Zurich, CH-8093 Zurich, Switzerland, 2Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 3INAF National Institute for Astrophysics, I-00136 Rome, Italy, 4Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 5Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 6Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 7Max-Planck-Institut für Physik, D-80805 München, Germany, 8Max-Planck-Institut für Physik, D-80805 München, Germany, 9Universidad Complutense, E-28040 Madrid, Spain, 10Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 11University of Łódź, PL-90236 Lodz, Poland, 12Deutsches Elektronen-Synchrotron, 13Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 14ETH Zurich, CH-8093 Zurich, Switzerland, 15Institut de Fisica d'Altes Energies, 16Universidad Complutense, E-28040 Madrid, Spain, 17INAF National Institute for Astrophysics, I-00136 Rome, Italy, 18Max-Planck-Institut für Physik, D-80805 München, Germany, 19Universität Würzburg, D-97074 Würzburg, Germany, 20Università di Padova and INFN, I-35131 Padova, Italy, 21INAF National Institute for Astrophysics, I-00136 Rome, Italy, 22Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 23Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 24Max-Planck-Institut für Physik, D-80805 München, Germany, 25Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 26Universidad Complutense, E-28040 Madrid, Spain, 27Institut de Fisica d'Altes Energies, 28INAF National Institute for Astrophysics, I-00136 Rome, Italy, 29Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 30Max-Planck-Institut für Physik, D-80805 München, Germany, 31Università di Padova and INFN, I-35131 Padova, Italy, 32Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 33Institute for Space Sciences, 34INAF National Institute for Astrophysics, I-00136 Rome, Italy, 35Universidad Complutense, E-28040 Madrid, Spain, 36Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 37Universität Würzburg, D-97074 Würzburg, Germany, 38Università di Padova and INFN, I-35131 Padova, Italy, 39Technische Universität Dortmund, D-44221 Dortmund, Germany, 40Universität Würzburg, D-97074 Würzburg, Germany, 41Technische Universität Dortmund, D-44221 Dortmund, Germany, 42Institut de Fisica d'Altes Energies, 43Universidad Complutense, E-28040 Madrid, Spain, 44Universidad Complutense, E-28040 Madrid, Spain, 45Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 46Technische Universität Dortmund, D-44221 Dortmund, Germany, 47Max-Planck-Institut für Physik, D-80805 München, Germany, 48Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 49Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 50Deutsches Elektronen-Synchrotron, 51Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 52Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain, 53INAF National Institute for Astrophysics, I-00136 Rome, Italy, 54Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 55Institut de Fisica d'Altes Energies, 56Deutsches Elektronen-Synchrotron, 57Institut de Fisica d'Altes Energies, 58Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 59Max-Planck-Institut für Physik, D-80805 München, Germany, 60Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 61Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 62Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 63Max-Planck-Institut für Physik, D-80805 München, Germany, 64Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 65ETH Zurich, CH-8093 Zurich, Switzerland, 66University of Łódź, PL-90236 Lodz, Poland, 67Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 68Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 69Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 70Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 71INAF National Institute for Astrophysics, I-00136 Rome, Italy, 72Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 73Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 74INAF National Institute for Astrophysics, I-00136 Rome, Italy, 75Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 76Universidad Complutense, E-28040 Madrid, Spain, 77Institut de Fisica d'Altes Energies, 78Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata 700064, India, 79Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 80Deutsches Elektronen-Synchrotron, 81Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 82Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 83Universität Würzburg, D-97074 Würzburg, Germany, 84INAF National Institute for Astrophysics, I-00136 Rome, Italy, 85Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 86Università di Padova and INFN, I-35131 Padova, Italy, 87Institut de Fisica d'Altes Energies, 88Max-Planck-Institut für Physik, D-80805 München, Germany, 89Max-Planck-Institut für Physik, D-80805 München, Germany, 90Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 91Max-Planck-Institut für Physik, D-80805 München, Germany, 92Institut de Fisica d'Altes Energies, 93Max-Planck-Institut für Physik, D-80805 München, Germany, 94Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 95Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 96University of Łódź, PL-90236 Lodz, Poland, 97Universidad Complutense, E-28040 Madrid, Spain, 98Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 99Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 100Max-Planck-Institut für Physik, D-80805 München, Germany, 101Institut de Fisica d'Altes Energies, 102Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 103Technische Universität Dortmund, D-44221 Dortmund, Germany, 104Università di Padova and INFN, I-35131 Padova, Italy, 105Institut de Fisica d'Altes Energies, 106Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 107Max-Planck-Institut für Physik, D-80805 München, Germany, 108Università di Siena, and INFN Pisa, I-53100 Siena, Italy, 109Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 110Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 111Deutsches Elektronen-Synchrotron, 112INAF National Institute for Astrophysics, I-00136 Rome, Italy, 113Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 114Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 115Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy, 116ETH Zurich, CH-8093 Zurich, Switzerland, 117Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 118Technische Universität Dortmund, D-44221 Dortmund, Germany, 119Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 120Institut de Fisica d'Altes Energies, 121Max-Planck-Institut für Physik, D-80805 München, Germany, 122Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 123Deutsches Elektronen-Synchrotron, 124Università di Padova and INFN, I-35131 Padova, Italy, 125Max-Planck-Institut für Physik, D-80805 München, Germany, 126Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy, 127Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 128University of Łódź, PL-90236 Lodz, Poland, 129Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 130University of Łódź, PL-90236 Lodz, Poland, 131INAF National Institute for Astrophysics, I-00136 Rome, Italy, 132Universität Würzburg, D-97074 Würzburg, Germany, 133Max-Planck-Institut für Physik, D-80805 München, Germany, 134Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Astronomy Division, University of Oulu, Finland, 135Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 136INAF National Institute for Astrophysics, I-00136 Rome, Italy, 137Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 138Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 139Università di Padova and INFN, I-35131 Padova, Italy, 140Max-Planck-Institut für Physik, D-80805 München, Germany, 141Technische Universität Dortmund, D-44221 Dortmund, Germany, 142ICREA and Institute for Space Sciences, 143Max-Planck-Institut für Physik, D-80805 München, Germany, 144Università di Udine, and INFN Trieste, I-33100 Udine, Italy, 145Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria, 146Max-Planck-Institut für Physik, D-80805 München, Germany, 147Institut de Fisica d'Altes Energies, 148Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain, 149Institute for Space Sciences, 150Universitat de Barcelona, ICC, IEEC-UB, E-08028 Barcelona, Spain, 151Astron. Inst., St.-Petersburg State Univ., Russia, 152Graduate Institute of Astronomy, National Central University, 300 Zhongda Rd, Zhongli 32001, Taoyuan, Taiwan, 153Pulkovo Observatory, St.-Petersburg, Russia, 154Agrupació Astronòmica de Sabadell, Spain, 155Astron. Inst., St.-Petersburg State Univ., Russia, 156Aalto University Metsähovi Radio Observatory, Metsähovintie 114, FI-02540 Kylmälä, Finland, 157School of Cosmic Physics, Dublin Institute For Advanced Studies, Ireland, 158Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia, 159Astron. Inst., St.-Petersburg State Univ., Russia, 160Graduate Institute of Astronomy, National Central University, 300 Zhongda Rd, Zhongli 32001, Taoyuan, Taiwan, 161Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia, 162Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia, 163Aalto University Metsähovi Radio Observatory, Metsähovintie 114, FI-02540 Kylmälä, Finland, 164Astron. Inst., St.-Petersburg State Univ., Russia, 165Astron. Inst., St.-Petersburg State Univ., Russia, 166Astron. Inst., St.-Petersburg State Univ., Russia, 167Circolo Astrofili Talmassons, Italy, 168Graduate Institute of Astronomy, National Central University, 300 Zhongda Rd, Zhongli 32001, Taoyuan, Taiwan, 169School of Physics, University College Dublin, Belfield, Dublin 4, Ireland, 170Astron. Inst., St.-Petersburg State Univ., Russia, 171Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia, 172INAF - Osservatorio Astrofisico di Torino, 10025 Pino Torinese, 173Agrupació Astronòmica de Sabadell, Spain, 174Department of Physics, University of Colorado, Denver, USA, 175Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia, 176Aalto University Metsähovi Radio Observatory, Metsähovintie 114, FI-02540 Kylmälä, Finland, 177Astron. Inst., St.-Petersburg State Univ., Russia, 178INAF - Osservatorio Astrofisico di Torino, 10025 Pino Torinese

We study the multi-band variability and correlations of the TeV blazar Mrk 421 on year time scales, which can bring additional insight on the processes responsible for its broadband emission. We observed Mrk 421 in the very high energy (VHE) gamma-ray range with the Cherenkov telescope MAGIC-I from March 2007 to June 2009 for a total of 96 hours of effective time after quality cuts. The VHE flux variability is quantified with several methods, including the Bayesian Block algorithm, which is applied to data from Cherenkov telescopes for the first time. Read More

We present a complete optoelectronic unit for polarization visualization, switching and control. The system is based on an FPGA unit and comprises: an acquisition unit containing an analog polarimeter and digital-to-analog converters, an FPGA capable of implementing an optimal algorithm for three-stage arbitrary polarization tracking, and an electronic driver with analog-to-digital converters capable of interfacing with Lithium-Niobate-based Polarization Controllers. The results, determined via simulation of real-parameter devices, show that fast polarization switch is achievable. Read More

We apply the Riccati-Pad\'{e} method and the Rayleigh-Ritz method with complex rotation to the study of the resonances of a one-dimensional well with two barriers. The model exhibits two different kinds of resonances and we calculate them by means of both approaches. While the Rayleigh-Ritz method reveals each set at a particular interval of rotation angles the Riccati Pad\'{e} method yields both of them as roots of the same Hankel determinants. Read More

2016Mar
Authors: The MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, P. Antoranz4, A. Babic5, B. Banerjee6, P. Bangale7, U. Barres de Almeida8, J. A. Barrio9, J. Becerra Gonzalez10, W. Bednarek11, E. Bernardini12, B. Biasuzzi13, A. Biland14, O. Blanch15, S. Bonnefoy16, G. Bonnoli17, F. Borracci18, T. Bretz19, E. Carmona20, A. Carosi21, A. Chatterjee22, R. Clavero23, P. Colin24, E. Colombo25, J. L. Contreras26, J. Cortina27, S. Covino28, P. Da Vela29, F. Dazzi30, A. De Angelis31, G. De Caneva32, B. De Lotto33, E. de Ona Wilhelmi34, C. Delgado Mendez35, F. Di Pierro36, D. Dominis Prester37, D. Dorner38, M. Doro39, S. Einecke40, D. Elsaesser41, A. Fernandez-Barral42, D. Fidalgo43, M. V. Fonseca44, L. Font45, K. Frantzen46, C. Fruck47, D. Galindo48, R. J. Garcia Lopez49, M. Garczarczyk50, D. Garrido Terrats51, M. Gaug52, P. Giammaria53, D. Glawion54, N. Godinovic55, A. Gonzalez Munoz56, D. Guberman57, Y. Hanabata58, M. Hayashida59, J. Herrera60, J. Hose61, D. Hrupec62, G. Hughes63, W. Idec64, K. Kodani65, Y. Konno66, H. Kubo67, J. Kushida68, A. La Barbera69, D. Lelas70, E. Lindfors71, S. Lombardi72, F. Longo73, M. Lopez74, R. Lopez-Coto75, A. Lopez-Oramas76, E. Lorenz77, P. Majumdar78, M. Makariev79, K. Mallot80, G. Maneva81, M. Manganaro82, K. Mannheim83, L. Maraschi84, B. Marcote85, M. Mariotti86, M. Martinez87, D. Mazin88, U. Menzel89, J. M. Miranda90, R. Mirzoyan91, A. Moralejo92, D. Nakajima93, V. Neustroev94, A. Niedzwiecki95, M. Nievas Rosillo96, K. Nilsson97, K. Nishijima98, K. Noda99, R. Orito100, A. Overkemping101, S. Paiano102, J. Palacio103, M. Palatiello104, D. Paneque105, R. Paoletti106, J. M. Paredes107, X. Paredes-Fortuny108, M. Persic109, J. Poutanen110, P. G. Prada Moroni111, E. Prandini112, I. Puljak113, R. Reinthal114, W. Rhode115, M. Ribo116, J. Rico117, J. Rodriguez Garcia118, S. Rugamer119, T. Saito120, K. Satalecka121, V. Scapin122, C. Schultz123, T. Schweizer124, S. N. Shore125, A. Sillanpaa126, J. Sitarek127, I. Snidaric128, D. Sobczynska129, A. Stamerra130, T. Steinbring131, M. Strzys132, L. Takalo133, H. Takami134, F. Tavecchio135, P. Temnikov136, T. Terzic137, D. Tescaro138, M. Teshima139, J. Thaele140, D. F. Torres141, T. Toyama142, A. Treves143, V. Verguilov144, I. Vovk145, J. E. Ward146, M. Will147, M. H. Wu148, R. Zanin149, F. Lucarelli, C. Pittori, S. Vercellone for the AGILE team, A. Berdyugin, M. T. Carini, A. Lahteenmaki, M. Pasanen, A. Pease, J. Sainio, M. Tornikoski, R. Walters
Affiliations: 1Eisenacher, 2Eisenacher, 3Eisenacher, 4Eisenacher, 5Eisenacher, 6Eisenacher, 7Eisenacher, 8Eisenacher, 9Eisenacher, 10Eisenacher, 11Eisenacher, 12Eisenacher, 13Eisenacher, 14Eisenacher, 15Eisenacher, 16Eisenacher, 17Eisenacher, 18Eisenacher, 19Eisenacher, 20Eisenacher, 21Eisenacher, 22Eisenacher, 23Eisenacher, 24Eisenacher, 25Eisenacher, 26Eisenacher, 27Eisenacher, 28Eisenacher, 29Eisenacher, 30Eisenacher, 31Eisenacher, 32Eisenacher, 33Eisenacher, 34Eisenacher, 35Eisenacher, 36Eisenacher, 37Eisenacher, 38Eisenacher, 39Eisenacher, 40Eisenacher, 41Eisenacher, 42Eisenacher, 43Eisenacher, 44Eisenacher, 45Eisenacher, 46Eisenacher, 47Eisenacher, 48Eisenacher, 49Eisenacher, 50Eisenacher, 51Eisenacher, 52Eisenacher, 53Eisenacher, 54Eisenacher, 55The MAGIC Collaboration, 56The MAGIC Collaboration, 57The MAGIC Collaboration, 58The MAGIC Collaboration, 59The MAGIC Collaboration, 60The MAGIC Collaboration, 61The MAGIC Collaboration, 62The MAGIC Collaboration, 63The MAGIC Collaboration, 64The MAGIC Collaboration, 65The MAGIC Collaboration, 66The MAGIC Collaboration, 67The MAGIC Collaboration, 68The MAGIC Collaboration, 69The MAGIC Collaboration, 70The MAGIC Collaboration, 71The MAGIC Collaboration, 72The MAGIC Collaboration, 73The MAGIC Collaboration, 74The MAGIC Collaboration, 75The MAGIC Collaboration, 76The MAGIC Collaboration, 77The MAGIC Collaboration, 78The MAGIC Collaboration, 79The MAGIC Collaboration, 80The MAGIC Collaboration, 81The MAGIC Collaboration, 82The MAGIC Collaboration, 83The MAGIC Collaboration, 84The MAGIC Collaboration, 85The MAGIC Collaboration, 86The MAGIC Collaboration, 87The MAGIC Collaboration, 88The MAGIC Collaboration, 89The MAGIC Collaboration, 90The MAGIC Collaboration, 91The MAGIC Collaboration, 92The MAGIC Collaboration, 93The MAGIC Collaboration, 94The MAGIC Collaboration, 95The MAGIC Collaboration, 96The MAGIC Collaboration, 97The MAGIC Collaboration, 98The MAGIC Collaboration, 99The MAGIC Collaboration, 100The MAGIC Collaboration, 101The MAGIC Collaboration, 102The MAGIC Collaboration, 103The MAGIC Collaboration, 104The MAGIC Collaboration, 105The MAGIC Collaboration, 106The MAGIC Collaboration, 107The MAGIC Collaboration, 108The MAGIC Collaboration, 109The MAGIC Collaboration, 110The MAGIC Collaboration, 111The MAGIC Collaboration, 112The MAGIC Collaboration, 113The MAGIC Collaboration, 114The MAGIC Collaboration, 115The MAGIC Collaboration, 116The MAGIC Collaboration, 117The MAGIC Collaboration, 118The MAGIC Collaboration, 119The MAGIC Collaboration, 120The MAGIC Collaboration, 121The MAGIC Collaboration, 122The MAGIC Collaboration, 123The MAGIC Collaboration, 124The MAGIC Collaboration, 125The MAGIC Collaboration, 126The MAGIC Collaboration, 127The MAGIC Collaboration, 128The MAGIC Collaboration, 129The MAGIC Collaboration, 130The MAGIC Collaboration, 131The MAGIC Collaboration, 132The MAGIC Collaboration, 133The MAGIC Collaboration, 134The MAGIC Collaboration, 135The MAGIC Collaboration, 136The MAGIC Collaboration, 137The MAGIC Collaboration, 138The MAGIC Collaboration, 139The MAGIC Collaboration, 140The MAGIC Collaboration, 141The MAGIC Collaboration, 142The MAGIC Collaboration, 143The MAGIC Collaboration, 144The MAGIC Collaboration, 145The MAGIC Collaboration, 146The MAGIC Collaboration, 147The MAGIC Collaboration, 148The MAGIC Collaboration, 149The MAGIC Collaboration

The BL Lac object 1ES 1011+496 was discovered at Very High Energy gamma-rays by MAGIC in spring 2007. Before that the source was little studied in different wavelengths. Therefore a multi-wavelength (MWL) campaign was organized in spring 2008. Read More

2016Mar
Authors: MAGIC Collaboration, M. L. Ahnen1, S. Ansoldi2, L. A. Antonelli3, P. Antoranz4, A. Babic5, B. Banerjee6, P. Bangale7, U. Barres de Almeida8, J. A. Barrio9, J. Becerra González10, W. Bednarek11, E. Bernardini12, B. Biasuzzi13, A. Biland14, O. Blanch15, S. Bonnefoy16, G. Bonnoli17, F. Borracci18, T. Bretz19, S. Buson20, A. Carosi21, A. Chatterjee22, R. Clavero23, P. Colin24, E. Colombo25, J. L. Contreras26, J. Cortina27, S. Covino28, P. Da Vela29, F. Dazzi30, A. De Angelis31, B. De Lotto32, E. de Oña Wilhelmi33, C. Delgado Mendez34, F. Di Pierro35, A. Domínguez36, D. Dominis Prester37, D. Dorner38, M. Doro39, S. Einecke40, D. Eisenacher Glawion41, D. Elsaesser42, A. Fernández-Barral43, D. Fidalgo44, M. V. Fonseca45, L. Font46, K. Frantzen47, C. Fruck48, D. Galindo49, R. J. García López50, M. Garczarczyk51, D. Garrido Terrats52, M. Gaug53, P. Giammaria54, N. Godinović55, A. González Muñoz56, D. Gora57, D. Guberman58, D. Hadasch59, A. Hahn60, Y. Hanabata61, M. Hayashida62, J. Herrera63, J. Hose64, D. Hrupec65, G. Hughes66, W. Idec67, K. Kodani68, Y. Konno69, H. Kubo70, J. Kushida71, A. La Barbera72, D. Lelas73, E. Lindfors74, S. Lombardi75, F. Longo76, M. López77, R. López-Coto78, A. López-Oramas79, P. Majumdar80, M. Makariev81, K. Mallot82, G. Maneva83, M. Manganaro84, K. Mannheim85, L. Maraschi86, B. Marcote87, M. Mariotti88, M. Martínez89, D. Mazin90, U. Menzel91, J. M. Miranda92, R. Mirzoyan93, A. Moralejo94, E. Moretti95, D. Nakajima96, V. Neustroev97, A. Niedzwiecki98, M. Nievas Rosillo99, K. Nilsson100, K. Nishijima101, K. Noda102, R. Orito103, A. Overkemping104, S. Paiano105, J. Palacio106, M. Palatiello107, D. Paneque108, R. Paoletti109, J. M. Paredes110, X. Paredes-Fortuny111, G. Pedaletti112, M. Persic113, J. Poutanen114, P. G. Prada Moroni115, E. Prandini116, I. Puljak117, W. Rhode118, M. Ribó119, J. Rico120, J. Rodriguez Garcia121, T. Saito122, K. Satalecka123, C. Schultz124, T. Schweizer125, S. N. Shore126, A. Sillanpää127, J. Sitarek128, I. Snidaric129, D. Sobczynska130, A. Stamerra131, T. Steinbring132, M. Strzys133, L. Takalo134, H. Takami135, F. Tavecchio136, P. Temnikov137, T. Terzić138, D. Tescaro139, M. Teshima140, J. Thaele141, D. F. Torres142, T. Toyama143, A. Treves144, V. Verguilov145, I. Vovk146, J. E. Ward147, M. Will148, M. H. Wu149, R. Zanin150, J. Casares151, A. Herrero152
Affiliations: 1ETH Zurich, Switzerland, 2Università di Udine, and INFN Trieste, Italy, 3INAF National Institute for Astrophysics, Italy, 4Università di Siena, and INFN Pisa, Italy, 5Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 6Saha Institute of Nuclear Physics, India, 7Max-Planck-Institut für Physik, Germany, 8Max-Planck-Institut für Physik, Germany, 9Universidad Complutense, Spain, 10Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 11University of Łódź, Poland, 12Deutsches Elektronen-Synchrotron, 13Università di Udine, and INFN Trieste, Italy, 14ETH Zurich, Switzerland, 15Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 16Universidad Complutense, Spain, 17INAF National Institute for Astrophysics, Italy, 18Max-Planck-Institut für Physik, Germany, 19Universität Würzburg, Germany, 20Università di Padova and INFN, Italy, 21INAF National Institute for Astrophysics, Italy, 22Saha Institute of Nuclear Physics, India, 23Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 24Max-Planck-Institut für Physik, Germany, 25Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 26Universidad Complutense, Spain, 27Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 28INAF National Institute for Astrophysics, Italy, 29Università di Siena, and INFN Pisa, Italy, 30Max-Planck-Institut für Physik, Germany, 31Università di Padova and INFN, Italy, 32Università di Udine, and INFN Trieste, Italy, 33Institute for Space Sciences, 34Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Spain, 35INAF National Institute for Astrophysics, Italy, 36Universidad Complutense, Spain, 37Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 38Universität Würzburg, Germany, 39Università di Padova and INFN, Italy, 40Technische Universität Dortmund, Germany, 41Universität Würzburg, Germany, 42Universität Würzburg, Germany, 43Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 44Universidad Complutense, Spain, 45Universidad Complutense, Spain, 46Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Spain, 47Technische Universität Dortmund, Germany, 48Max-Planck-Institut für Physik, Germany, 49Universitat de Barcelona, ICC, IEEC-UB, Spain, 50Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 51Deutsches Elektronen-Synchrotron, 52Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Spain, 53Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, Spain, 54INAF National Institute for Astrophysics, Italy, 55Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 56Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 57Deutsches Elektronen-Synchrotron, 58Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 59Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 60Max-Planck-Institut für Physik, Germany, 61Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 62Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 63Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 64Max-Planck-Institut für Physik, Germany, 65Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 66ETH Zurich, Switzerland, 67University of Łódź, Poland, 68Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 69Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 70Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 71Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 72INAF National Institute for Astrophysics, Italy, 73Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 74Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland, 75INAF National Institute for Astrophysics, Italy, 76Università di Udine, and INFN Trieste, Italy, 77Universidad Complutense, Spain, 78Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 79Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 80Saha Institute of Nuclear Physics, India, 81Inst. for Nucl. Research and Nucl. Energy, Bulgaria, 82Deutsches Elektronen-Synchrotron, 83Inst. for Nucl. Research and Nucl. Energy, Bulgaria, 84Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 85Universität Würzburg, Germany, 86INAF National Institute for Astrophysics, Italy, 87Universitat de Barcelona, ICC, IEEC-UB, Spain, 88Università di Padova and INFN, Italy, 89Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 90Max-Planck-Institut für Physik, Germany, 91Max-Planck-Institut für Physik, Germany, 92Università di Siena, and INFN Pisa, Italy, 93Max-Planck-Institut für Physik, Germany, 94Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 95Max-Planck-Institut für Physik, Germany, 96Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 97Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland, 98University of Łódź, Poland, 99Universidad Complutense, Spain, 100Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland, 101Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 102Max-Planck-Institut für Physik, Germany, 103Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 104Technische Universität Dortmund, Germany, 105Università di Padova and INFN, Italy, 106Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 107Università di Udine, and INFN Trieste, Italy, 108Max-Planck-Institut für Physik, Germany, 109Università di Siena, and INFN Pisa, Italy, 110Universitat de Barcelona, ICC, IEEC-UB, Spain, 111Universitat de Barcelona, ICC, IEEC-UB, Spain, 112Deutsches Elektronen-Synchrotron, 113Università di Udine, and INFN Trieste, Italy, 114Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland, 115Università di Pisa, and INFN Pisa, Italy, 116ETH Zurich, Switzerland, 117Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 118Technische Universität Dortmund, Germany, 119Universitat de Barcelona, ICC, IEEC-UB, Spain, 120Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 121Max-Planck-Institut für Physik, Germany, 122Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 123Universidad Complutense, Spain, 124Università di Padova and INFN, Italy, 125Max-Planck-Institut für Physik, Germany, 126Università di Pisa, and INFN Pisa, Italy, 127Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland, 128University of Łódź, Poland, 129Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 130University of Łódź, Poland, 131INAF National Institute for Astrophysics, Italy, 132Universität Würzburg, Germany, 133Max-Planck-Institut für Physik, Germany, 134Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland, 135Japanese MAGIC Consortium, ICRR, The University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, The University of Tokushima, KEK, Japan, 136INAF National Institute for Astrophysics, Italy, 137Inst. for Nucl. Research and Nucl. Energy, Bulgaria, 138Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka, University of Split and University of Zagreb, Croatia, 139Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 140Max-Planck-Institut für Physik, Germany, 141Technische Universität Dortmund, Germany, 142ICREA and Institute for Space Sciences, 143Max-Planck-Institut für Physik, Germany, 144Università di Udine, and INFN Trieste, Italy, 145Inst. for Nucl. Research and Nucl. Energy, Bulgaria, 146Max-Planck-Institut für Physik, Germany, 147Institut de Fisica d'Altes Energies, The Barcelona Institute of Science and Technology, 148Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 149Institute for Space Sciences, 150Universitat de Barcelona, ICC, IEEC-UB, Spain, 151Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain, 152Inst. de Astrofísica de Canarias, Universidad de La Laguna, Spain

The gamma-ray binary LS I +61$^{\circ}$303 is a well established source from centimeter radio up to very high energy (VHE; E$>$100 GeV). Its broadband emission shows a periodicity of $\sim$26.5 days, coincident with the orbital period. Read More