M. Krause - Excellence Cluster Universe

M. Krause
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M. Krause
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Excellence Cluster Universe
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High Energy Astrophysical Phenomena (33)
 
Astrophysics of Galaxies (11)
 
Instrumentation and Methods for Astrophysics (8)
 
High Energy Physics - Phenomenology (3)
 
Cosmology and Nongalactic Astrophysics (2)
 
Solar and Stellar Astrophysics (2)
 
Physics - Instrumentation and Detectors (2)
 
Physics - Physics Education (1)
 
High Energy Physics - Experiment (1)
 
Nonlinear Sciences - Adaptation and Self-Organizing Systems (1)
 
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Publications Authored By M. Krause

2017May
Affiliations: 1Florida Tech, 2UMBC, 3UMass, 4Purple Mtn. Obs., 5Queens, 6Queens, 7MPIfR, 8Queens, 9Caltech, 10Kapetyn Inst., 11Ruhr-Universitat Bochum

Tidal disruption events (TDEs) occur when a star or sub-stellar object passes close enough to a galaxy's supermassive black hole to be disrupted by tidal forces. NGC 4845 (d=17 Mpc) was host to a TDE, IGR J12580+0134, detected in November 2010. Its proximity offers us a unique close-up of the TDE and its aftermath. Read More

2017Mar
Affiliations: 1Physics Department, McGill University, Montreal, 2Department of Physics, Washington University, St. Louis, MO, 3Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ, 4Department of Physics and Astronomy, University of California, Los Angeles, CA, 5Physics Department, McGill University, Montreal, 6Department of Physics and Astronomy, Iowa State University, Ames, IA, 7Department of Physics and Astronomy, University of California, Los Angeles, CA, 8Department of Physics, Washington University, St. Louis, MO, 9Department of Physics, Washington University, St. Louis, MO, 10Argonne National Laboratory, Argonne, IL, 11Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ, 12Physics Department, California Polytechnic State University, San Luis Obispo, CA, 13School of Physics, National University of Ireland Galway, University Road, Galway, Ireland, 14Department of Physics and Astronomy, Purdue University, West Lafayette, IN, 15Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ, 16Physics Department, McGill University, Montreal, 17Department of Physics and Astronomy, Purdue University, West Lafayette, IN, 18DESY, Zeuthen, Germany, 19School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, 20Department of Physics, California State University - East Bay, Hayward, CA, 21Department of Physics, Brown University, Providence, RI, 22Physics Department, McGill University, Montreal, 23Department of Physics, Stevens Institute of Technology, Hoboken, NJ, 24DESY, Zeuthen, Germany, 25Institute of Physics and Astronomy, University of Potsdam, Germany, 26Physics Department, McGill University, Montreal, 27Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA, 28Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE, 29Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ, 30Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA, 31Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA, 32Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, 33DESY, Zeuthen, Germany, 34Department of Physics and Astronomy, DePauw University, Greencastle, IN, 35Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, 36Department of Physics, Brown University, Providence, RI, 37DESY, Zeuthen, Germany, 38Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE, 39School of Physics, National University of Ireland Galway, University Road, Galway, Ireland, 40Physics Department, McGill University, Montreal, 41Department of Physics and Astronomy, Purdue University, West Lafayette, IN, 42School of Physics, National University of Ireland Galway, University Road, Galway, Ireland, 43Physics Department, Columbia University, New York, NY, 44School of Physics, University College Dublin, Ireland, 45Department of Physics and Astronomy, University of California, Los Angeles, CA, 46School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, 47Enrico Fermi Institute, University of Chicago, Chicago, IL, 48Institute of Physics and Astronomy, University of Potsdam, Germany, 49Department of Physics and Astronomy, University of California, Los Angeles, CA, 50DESY, Zeuthen, Germany, 51School of Physics, University College Dublin, Ireland, 52Physics Department, McGill University, Montreal, 53Department of Physical Sciences, Cork Institute of Technology, Cork, Ireland, 54School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, 55Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ, 56School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, 57DESY, Zeuthen, Germany, 58Department of Physics and Astronomy, Barnard College, Columbia University, NY, 59Department of Physics and Astronomy, Purdue University, West Lafayette, IN, 60School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, 61University of Maryland, College Park / NASA GSFC, College Park, MD, 62Enrico Fermi Institute, University of Chicago, Chicago, IL, 63Institute of Physics and Astronomy, University of Potsdam, Germany, 64Physics Department, McGill University, Montreal, 65Department of Physics and Astronomy, Purdue University, West Lafayette, IN, 66Physics Department, McGill University, Montreal, 67Enrico Fermi Institute, University of Chicago, Chicago, IL, 68Department of Physics and Astronomy, Iowa State University, Ames, IA, 69Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA, 70Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA, 71Physics Department, McGill University, Montreal

We present constraints on the annihilation cross section of WIMP dark matter based on the joint statistical analysis of four dwarf galaxies with VERITAS. These results are derived from an optimized photon weighting statistical technique that improves on standard imaging atmospheric Cherenkov telescope (IACT) analyses by utilizing the spectral and spatial properties of individual photon events. We report on the results of $\sim$230 hours of observations of five dwarf galaxies and the joint statistical analysis of four of the dwarf galaxies. Read More

Imaging atmospheric Cherenkov telescopes (IACTs) are equipped with sensitive photomultiplier tube (PMT) cameras. Exposure to high levels of background illumination degrades the efficiency of and potentially destroys these photo-detectors over time, so IACTs cannot be operated in the same configuration in the presence of bright moonlight as under dark skies. Since September 2012, observations have been carried out with the VERITAS IACTs under bright moonlight (defined as about three times the night-sky-background (NSB) of a dark extragalactic field, typically occurring when Moon illumination > 35%) in two observing modes, firstly by reducing the voltage applied to the PMTs and, secondly, with the addition of ultra-violet (UV) bandpass filters to the cameras. Read More

80% of all Renewable Energy Power in Germany is installed in tree-like distribution grids. Intermittent power fluctuations from such sources introduce new dynamics into the lower grid layers. At the same time, distributed resources will have to contribute to stabilize the grid against these fluctuations in the future. Read More

2017Feb
Authors: M. G. Aartsen, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, I. Al Samarai, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arg/"uelles, 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, E. Blaufuss, S. Blot, C. Bohm, M. Börner, F. Bos, D. Bose, S. Böser, 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 André, 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, 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. Fösig, A. Franckowiak, E. Friedman, T. Fuchs, T. K. Gaisser, J. Gallagher, L. Gerhardt, K. Ghorbani, W. Giang, L. Gladstone, T. Glauch, T. Glüsenkamp, A. Goldschmidt, J. G. Gonzalez, D. Grant, Z. Griffith, C. Haack, 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. Hoshina, F. Huang, M. Huber, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, W. Kang, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, A. Kheirandish, J. Kim, M. Kim, T. Kintscher, J. Kiryluk, T. Kittler, S. R. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, M. Kroll, G. Krückl, C. Krüger, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, A. Kyriacou, M. Labare, J. L. Lanfranchi, M. J. Larson, F. Lauber, M. Lesiak-Bzdak, M. Leuermann, L. Lu, J. Lünemann, 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, T. Menne, G. Merino, T. Meures, S. Miarecki, J. Micallef, G. Momenté, 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, Ö. Penek, J. A. Pepper, C. Pérez de los Heros, D. Pieloth, E. Pinat, P. B. Price, G. T. Przybylski, M. Quinnan, C. Raab, L. Rädel, 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. Schöneberg, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, J. Stachurska, T. Stanev, A. Stasik, J. Stettner, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, R. Ström, N. L. Strotjohann, G. W. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, F. Tenholt, S. Ter-Antonyan, A. Terliuk, G. Tešić, S. Tilav, P. A. Toale, M. N. Tobin, S. Toscano, D. Tosi, M. Tselengidou, C. F. Tung, A. Turcati, E. Unger, M. Usner, J. Vandenbroucke, N. van Eijndhoven, S. Vanheule, M. van Rossem, J. van Santen, M. Vehring, M. Voge, E. Vogel, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, A. Waza, 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, K. Z. Stanek, B. J. Shappee, C. S. Kochanek, T. W. -S. Holoien, J. L. Prieto, D. B. Fox, J. J. DeLaunay, C. F. Turley, S. D. Barthelmy, A. Y. Lien, P. Mészáros, K. Murase, D. Kocevski, R. Buehler, M. Giomi, J. L. Racusin, A. Albert, R. Alfaro, C. Alvarez, J. D. Álvarez, R. Arceo, J. C. Arteaga-Velázquez, H. A. Ayala Solares, E. Belmont-Moreno, A. Bernal, C. Brisbois, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, M. Castillo, U. Cotti, E. de la Fuente, S. Coutino de León, C. De León, R. Diaz Hernandez, B. L. Dingus, M. A. DuVernois, J. C. Díaz-Vélez, D. W. Fiorino, N. Fraija, J. A. García-González, M. Gerhardt, A. González Muñoz, M. M. González, J. A. Goodman, Z. Hampel-Arias, J. P. Harding, S. Hernandez, C. M. Hui, P. Hüntemeyer, A. Iriarte, A. Jardin-Blicq, V. Joshi, S. Kaufmann, A. Lara, R. J. Lauer, W. H. Lee, D. Lennarz, H. León Vargas, J. T. Linnemann, G. Luis Raya, R. Luna-García, R. López-Coto, K. Malone, S. S. Marinelli, O. Martinez, I. Martinez-Castellanos, J. Martínez-Castro, H. Martínez-Huerta, J. A. Matthews, E. Moreno, M. Mostafá, L. Nellen, M. Newbold, M. U. Nisa, R. Pelayo, J. Pretz, E. G. Pérez-Pérez, Z. Ren, C. D. Rho, C. Rivière, D. Rosa-González, M. Rosenberg, F. Salesa Greus, A. Sandoval, M. Schneider, H. Schoorlemmer, G. Sinnis, A. J. Smith, R. W. Springer, P. Surajbali, O. Tibolla, K. Tollefson, I. Torres, L. Villaseñor, T. Weisgarber, I. G. Wisher, J. Wood, T. Yapici, A. Zepeda, H. Zhou, I. Arcavi, G. Hosseinzadeh, D. A. Howell, S. Valenti, C. McCully, V. M. Lipunov, E. S. Gorbovskoy, N. V. Tiurina, P. V. Balanutsa, A. S. Kuznetsov, V. G. Kornilov, V. Chazov, N. M. Budnev, O. A. Gress, K. I. Ivanov, A. G. Tlatov, R. Rebolo Lopez, M. Serra-Ricart, P. A. Evans, J. A. Kennea, N. Gehrels, J. P. Osborne, K. L. Page, A. U. Abeysekara, A. Archer, W. Benbow, R. Bird, T. Brantseg, V. Bugaev, J. V Cardenzana, M. P. Connolly, W. Cui, A. Falcone, Q. Feng, J. P. Finley, H. Fleischhack, L. Fortson, A. Furniss, S. Griffin, J. Grube, M. Hütten, O. Hervet, J. Holder, G. Hughes, T. B. Humensky, C. A. Johnson, P. Kaaret, P. Kar, N. Kelley-Hoskins, M. Kertzman, M. Krause, S. Kumar, M. J. Lang, T. T. Y. Lin, S. McArthur, P. Moriarty, R. Mukherjee, D. Nieto, R. A. Ong, A. N. Otte, 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, D. Staszak, S. Trépanier, J. Tyler, S. P. Wakely, A. Weinstein, P. Wilcox, A. Wilhelm, D. A. Williams, B. Zitzer, E. Bellm, Z. Cano, A. Gal-Yam, D. A. Kann, E. O. Ofek, M. Rigault, M. Soumagnac

On February 17 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of each other which are consistent with a point source origin. Such a triplet is expected only once every 13.7 years as a random coincidence of background events. Read More

High-energy gamma-ray emission from supernova remnants (SNRs) has provided a unique perspective for studies of Galactic cosmic-ray acceleration. Tycho's SNR is a particularly good target because it is a young, type Ia SNR that is well-studied over a wide range of energies and located in a relatively clean environment. Since the detection of gamma-ray emission from Tycho's SNR by VERITAS and Fermi-LAT, there have been several theoretical models proposed to explain its broadband emission and high-energy morphology. Read More

Imaging atmospheric Cherenkov telescopes record an enormous number of cosmic-ray background events. Suppressing these background events while retaining $\gamma$-rays is key to achieving good sensitivity to faint $\gamma$-ray sources. The differentiation between signal and background events can be accomplished using machine learning algorithms, which are already used in various fields of physics. Read More

Computing polarised intensities from noisy data in Stokes U and Q suffers from a positive bias that should be suppressed. To develop a correction method that, when applied to maps, should provide a distribution of polarised intensity that closely follows the signal from the source. We propose a new method to suppress the bias by estimating the polarisation angle of the source signal in a noisy environment with help of a modified median filter. Read More

B2 1215+30 is a BL Lac-type blazar that was first detected at TeV energies by the MAGIC atmospheric Cherenkov telescopes, and subsequently confirmed by the VERITAS observatory with data collected between 2009 and 2012. In 2014 February 08, VERITAS detected a large-amplitude flare from B2 1215+30 during routine monitoring observations of the blazar 1ES 1218+304, located in the same field of view. The TeV flux reached 2. Read More

We present a search for magnetically broadened gamma-ray emission around active galactic nuclei (AGN), using VERITAS observations of seven hard-spectrum blazars. A cascade process occurs when multi-TeV gamma rays from AGN interact with extragalactic background light (EBL) photons to produce electron-positron pairs, which then interact with cosmic microwave background (CMB) photons via inverse-Compton scattering to produce gamma rays. Due to the deflection of the electron-positron pairs, a non-zero intergalactic magnetic field (IGMF) would potentially produce detectable effects on the angular distribution of the cascade emission. 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

The discovery of the Higgs boson by the LHC experiments ATLAS and CMS has marked a milestone for particle physics. Yet, there are still many open questions that cannot be answered within the Standard Model (SM). For example, the generation of the observed matter-antimatter asymmetry in the universe through baryogenesis can only be explained qualitatively in the SM. 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 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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

We study the spectral energy distribution (SED) of the radio continuum emission from the KINGFISH sample of nearby galaxies to understand the energetics and origin of this emission. Effelsberg multi-wavelength observations at 1.4GHz, 4. Read More

2016Oct
Authors: The CTA Consortium, :, A. Abchiche, U. Abeysekara, Ó. Abril, F. Acero, B. S. Acharya, C. Adams, G. Agnetta, F. Aharonian, A. Akhperjanian, A. Albert, M. Alcubierre, J. Alfaro, R. Alfaro, A. J. Allafort, R. Aloisio, J. -P. Amans, E. Amato, L. Ambrogi, G. Ambrosi, M. Ambrosio, J. Anderson, M. Anduze, E. O. Angüner, E. Antolini, L. A. Antonelli, M. Antonucci, V. Antonuccio, P. Antoranz, C. Aramo, A. Aravantinos, M. Araya, C. Arcaro, B. Arezki, A. Argan, T. Armstrong, F. Arqueros, L. Arrabito, M. Arrieta, K. Asano, M. Ashley, P. Aubert, C. B. Singh, A. Babic, M. Backes, A. Bais, S. Bajtlik, C. Balazs, M. Balbo, D. Balis, C. Balkowski, O. Ballester, J. Ballet, A. Balzer, A. Bamba, R. Bandiera, A. Barber, C. Barbier, M. Barcelo, M. Barkov, A. Barnacka, U. Barres de Almeida, J. A. Barrio, S. Basso, D. Bastieri, C. Bauer, U. Becciani, Y. Becherini, J. Becker Tjus, V. Beckmann, W. Bednarek, W. Benbow, D. Benedico Ventura, J. Berdugo, D. Berge, E. Bernardini, M. G. Bernardini, S. Bernhard, K. Bernlöhr, B. Bertucci, M. -A. Besel, V. Beshley, N. Bhatt, P. Bhattacharjee, W. Bhattacharyya, S. Bhattachryya, B. Biasuzzi, G. Bicknell, C. Bigongiari, A. Biland, A. Bilinsky, W. Bilnik, B. Biondo, R. Bird, T. Bird, E. Bissaldi, M. Bitossi, O. Blanch, P. Blasi, J. Blazek, C. Bockermann, C. Boehm, L. Bogacz, M. Bogdan, M. Bohacova, C. Boisson, J. Boix, J. Bolmont, G. Bonanno, A. Bonardi, C. Bonavolontà, P. Bonifacio, F. Bonnarel, G. Bonnoli, J. Borkowski, R. Bose, Z. Bosnjak, M. Böttcher, J. -J. Bousquet, C. Boutonnet, F. Bouyjou, L. Bowman, C. Braiding, T. Brantseg, S. Brau-Nogué, J. Bregeon, M. Briggs, M. Brigida, T. Bringmann, W. Brisken, D. Bristow, R. Britto, E. Brocato, S. Bron, P. Brook, W. Brooks, A. M. Brown, K. Brügge, F. Brun, P. Brun, P. Brun, G. Brunetti, L. Brunetti, P. Bruno, T. Buanes, N. Bucciantini, G. Buchholtz, J. Buckley, V. Bugaev, R. Bühler, A. Bulgarelli, T. Bulik, M. Burton, A. Burtovoi, G. Busetto, S. Buson, J. Buss, K. Byrum, F. Cadoux, J. Calvo Tovar, R. Cameron, F. Canelli, R. Canestrari, M. Capalbi, M. Capasso, G. Capobianco, A. Caproni, P. Caraveo, J. Cardenzana, M. Cardillo, S. Carius, C. Carlile, A. Carosi, R. Carosi, E. Carquín, J. Carr, M. Carroll, J. Carter, P. -H. Carton, J. -M. Casandjian, S. Casanova, S. Casanova, E. Cascone, M. Casiraghi, A. Castellina, J. Castroviejo Mora, F. Catalani, O. Catalano, S. Catalanotti, D. Cauz, S. Cavazzani, P. Cerchiara, E. Chabanne, P. Chadwick, T. Chaleil, C. Champion, A. Chatterjee, S. Chaty, R. Chaves, A. Chen, X. Chen, X. Chen, K. Cheng, M. Chernyakova, L. Chiappetti, M. Chikawa, D. Chinn, V. R. Chitnis, N. Cho, A. Christov, J. Chudoba, M. Cieślar, M. A. Ciocci, R. Clay, S. Colafrancesco, P. Colin, J. -M. Colley, E. Colombo, J. Colome, S. Colonges, V. Conforti, V. Connaughton, S. Connell, J. Conrad, J. L. Contreras, P. Coppi, S. Corbel, J. Coridian, R. Cornat, P. Corona, D. Corti, J. Cortina, L. Cossio, A. Costa, H. Costantini, G. Cotter, B. Courty, S. Covino, G. Covone, G. Crimi, S. J. Criswell, R. Crocker, J. Croston, J. Cuadra, P. Cumani, G. Cusumano, P. Da Vela, Ø. Dale, F. D'Ammando, D. Dang, V. T. Dang, L. Dangeon, M. Daniel, I. Davids, I. Davids, B. Dawson, F. Dazzi, B. de Aguiar Costa, A. De Angelis, R. F. de Araujo Cardoso, V. De Caprio, R. de Cássia dos Anjos, G. De Cesare, A. De Franco, F. De Frondat, E. M. de Gouveia Dal Pino, I. de la Calle, C. De Lisio, R. de los Reyes Lopez, B. De Lotto, A. De Luca, J. R. T. de Mello Neto, M. de Naurois, E. de Oña Wilhelmi, F. De Palma, F. De Persio, V. de Souza, G. Decock, J. Decock, C. Deil, M. Del Santo, E. Delagnes, G. Deleglise, C. Delgado, J. Delgado, D. della Volpe, P. Deloye, M. Detournay, A. Dettlaff, J. Devin, T. Di Girolamo, C. Di Giulio, A. Di Paola, F. Di Pierro, M. A. Diaz, C. Díaz, C. Dib, J. Dick, H. Dickinson, S. Diebold, S. Digel, J. Dipold, G. Disset, A. Distefano, A. Djannati-Ataï, M. Doert, M. Dohmke, A. Domínguez, N. Dominik, J. -L. Dominique, D. Dominis Prester, A. Donat, I. Donnarumma, D. Dorner, M. Doro, J. -L. Dournaux, T. Downes, K. Doyle, G. Drake, S. Drappeau, H. Drass, D. Dravins, L. Drury, G. Dubus, L. Ducci, D. Dumas, K. Dundas Morå, D. Durand, D. D'Urso, V. Dwarkadas, J. Dyks, M. Dyrda, J. Ebr, E. Edy, K. Egberts, P. Eger, A. Egorov, S. Einecke, J. Eisch, F. Eisenkolb, C. Eleftheriadis, D. Elsaesser, D. Elsässer, D. Emmanoulopoulos, C. Engelbrecht, D. Engelhaupt, J. -P. Ernenwein, P. Escarate, S. Eschbach, C. Espinoza, P. Evans, M. Fairbairn, D. Falceta-Goncalves, A. Falcone, V. Fallah Ramazani, D. Fantinel, K. Farakos, C. Farnier, E. Farrell, G. Fasola, Y. Favre, E. Fede, R. Fedora, E. Fedorova, S. Fegan, D. Ferenc, M. Fernandez-Alonso, A. Fernández-Barral, G. Ferrand, O. Ferreira, M. Fesquet, P. Fetfatzis, E. Fiandrini, A. Fiasson, A. Filipčič, M. Filipovic, D. Fink, C. Finley, J. P. Finley, A. Finoguenov, V. Fioretti, M. Fiorini, H. Fleischhack, H. Flores, D. Florin, C. Föhr, E. Fokitis, M. V. Fonseca, L. Font, G. Fontaine, B. Fontes, M. Fornasa, M. Fornasa, A. Förster, P. Fortin, L. Fortson, N. Fouque, A. Franckowiak, A. Franckowiak, F. J. Franco, I. Freire Mota Albuquerque, L. Freixas Coromina, L. Fresnillo, C. Fruck, M. Fuessling, D. Fugazza, Y. Fujita, S. Fukami, Y. Fukazawa, T. Fukuda, Y. Fukui, S. Funk, A. Furniss, W. Gäbele, S. Gabici, A. Gadola, D. Galindo, D. D. Gall, Y. Gallant, D. Galloway, S. Gallozzi, J. A. Galvez, S. Gao, A. Garcia, B. Garcia, R. García Gil, R. Garcia López, M. Garczarczyk, D. Gardiol, C. Gargano, F. Gargano, S. Garozzo, F. Garrecht, L. Garrido, M. Garrido-Ruiz, D. Gascon, J. Gaskins, J. Gaudemard, M. Gaug, J. Gaweda, B. Gebhardt, M. Gebyehu, N. Geffroy, B. Genolini, L. Gerard, A. Ghalumyan, A. Ghedina, P. Ghislain, P. Giammaria, E. Giannakaki, F. Gianotti, S. Giarrusso, G. Giavitto, B. Giebels, T. Gieras, N. Giglietto, V. Gika, R. Gimenes, M. Giomi, P. Giommi, F. Giordano, G. Giovannini, P. Girardot, E. Giro, M. Giroletti, J. Gironnet, A. Giuliani, J. -F. Glicenstein, R. Gnatyk, N. Godinovic, P. Goldoni, G. Gomez, M. M. Gonzalez, A. González, D. Gora, K. S. Gothe, D. Gotz, J. Goullon, T. Grabarczyk, R. Graciani, J. Graham, P. Grandi, J. Granot, G. Grasseau, R. Gredig, A. J. Green, A. M. Green, T. Greenshaw, I. Grenier, S. Griffiths, A. Grillo, M. -H. Grondin, J. Grube, M. Grudzinska, J. Grygorczuk, V. Guarino, D. Guberman, S. Gunji, G. Gyuk, D. Hadasch, A. Hagedorn, L. Hagge, J. Hahn, H. Hakobyan, S. Hara, M. J. Hardcastle, T. Hassan, K. Hatanaka, T. Haubold, A. Haupt, T. Hayakawa, M. Hayashida, M. Heller, R. Heller, J. C. Helo, F. Henault, G. Henri, G. Hermann, R. Hermel, J. Herrera Llorente, J. Herrera Llorente, A. Herrero, O. Hervet, N. Hidaka, J. Hinton, W. Hirai, K. Hirotani, B. Hnatyk, J. Hoang, D. Hoffmann, W. Hofmann, T. Holch, J. Holder, S. Hooper, D. Horan, J. Hörandel, M. Hörbe, D. Horns, P. Horvath, J. Hose, J. Houles, T. Hovatta, M. Hrabovsky, D. Hrupec, J. -M. Huet, M. Huetten, G. Hughes, D. Hui, T. B. Humensky, M. Hussein, M. Iacovacci, A. Ibarra, Y. Ikeno, J. M. Illa, D. Impiombato, T. Inada, S. Incorvaia, L. Infante, Y. Inome, S. Inoue, T. Inoue, Y. Inoue, F. Iocco, K. Ioka, M. Iori, K. Ishio, K. Ishio, G. L. Israel, Y. Iwamura, C. Jablonski, A. Jacholkowska, J. Jacquemier, M. Jamrozy, P. Janecek, M. Janiak, D. Jankowsky, F. Jankowsky, P. Jean, I. Jegouzo, P. Jenke, J. J. Jimenez, M. Jingo, M. Jingo, L. Jocou, T. Jogler, C. A. Johnson, M. Jones, M. Josselin, L. Journet, I. Jung, P. Kaaret, M. Kagaya, J. Kakuwa, O. Kalekin, C. Kalkuhl, H. Kamon, R. Kankanyan, A. Karastergiou, K. Kärcher, M. Karczewski, S. Karkar, P. Karn, J. Kasperek, H. Katagiri, J. Kataoka, K. Katarzyński, S. Kato, U. Katz, N. Kawanaka, L. Kaye, D. Kazanas, N. Kelley-Hoskins, J. Kersten, B. Khélifi, D. B. Kieda, T. Kihm, S. Kimeswenger, S. Kisaka, S. Kishida, R. Kissmann, S. Klepser, W. Kluźniak, J. Knapen, J. Knapp, J. Knödlseder, B. Koch, F. Köck, J. Kocot, K. Kohri, K. Kokkotas, K. Kokkotas, D. Kolitzus, N. Komin, I. Kominis, A. Kong, Y. Konno, K. Kosack, G. Koss, M. Kossatz, G. Kowal, S. Koyama, J. Kozioł, M. Kraus, J. Krause, M. Krause, H. Krawzcynski, F. Krennrich, A. Kretzschmann, P. Kruger, H. Kubo, V. Kudryavtsev, G. Kukec Mezek, M. Kuklis, H. Kuroda, J. Kushida, A. La Barbera, N. La Palombara, V. La Parola, G. La Rosa, H. Laffon, R. Lahmann, M. Lakicevic, K. Lalik, G. Lamanna, D. Landriu, H. Landt, R. G. Lang, J. Lapington, P. Laporte, J. -P. Le Fèvre, T. Le Flour, P. Le Sidaner, S. -H. Lee, W. H. Lee, J. -P. Lees, J. Lefaucheur, K. Leffhalm, H. Leich, M. A. Leigui de Oliveira, D. Lelas, A. Lemière, M. Lemoine-Goumard, J. -P. Lenain, R. Leonard, R. Leoni, L. Lessio, G. Leto, A. Leveque, B. Lieunard, M. Limon, R. Lindemann, E. Lindfors, L. Linhoff, A. Liolios, A. Lipniacka, H. Lockart, T. Lohse, E. Łokas, S. Lombardi, F. Longo, A. Lopatin, M. Lopez, D. Loreggia, T. Louge, F. Louis, M. Louys, F. Lucarelli, D. Lucchesi, H. Lüdecke, T. Luigi, P. L. Luque-Escamilla, E. Lyard, M. C. Maccarone, T. Maccarone, T. J. Maccarone, E. Mach, G. M. Madejski, A. Madonna, F. Magniette, A. Magniez, M. Mahabir, G. Maier, P. Majumdar, P. Majumdar, M. Makariev, G. Malaguti, G. Malaspina, A. K. Mallot, A. Malouf, S. Maltezos, D. Malyshev, A. Mancilla, D. Mandat, G. Maneva, M. Manganaro, S. Mangano, P. Manigot, N. Mankushiyil, K. Mannheim, N. Maragos, D. Marano, P. Marchegiani, J. A. Marcomini, A. Marcowith, M. Mariotti, M. Marisaldi, S. Markoff, C. Martens, J. Martí, J. -M. Martin, L. Martin, P. Martin, G. Martínez, M. Martínez, O. Martínez, K. Martynyuk-Lototskyy, R. Marx, N. Masetti, P. Massimino, A. Mastichiadis, S. Mastroianni, M. Mastropietro, S. Masuda, H. Matsumoto, S. Matsuoka, N. Matthews, S. Mattiazzo, G. Maurin, N. Maxted, N. Maxted, J. Maya, M. Mayer, D. Mazin, M. N. Mazziotta, L. Mc Comb, N. McCubbin, I. McHardy, C. Medina, F. Mehrez, C. Melioli, D. Melkumyan, T. Melse, S. Mereghetti, M. Merk, P. Mertsch, J. -L. Meunier, T. Meures, M. Meyer, J. L. Meyrelles jr, A. Miccichè, T. Michael, J. Michałowski, P. Mientjes, I. Mievre, A. Mihailidis, J. Miller, T. Mineo, M. Minuti, N. Mirabal, F. Mirabel, J. M. Miranda, R. Mirzoyan, A. Mitchell, T. Mizuno, R. Moderski, I. Mognet, M. Mohammed, R. Moharana, L. Mohrmann, E. Molinari, P. Molyneux, E. Monmarthe, G. Monnier, T. Montaruli, C. Monte, I. Monteiro, D. Mooney, P. Moore, A. Moralejo, C. Morello, E. Moretti, K. Mori, P. Morris, A. Morselli, F. Moscato, D. Motohashi, F. Mottez, Y. Moudden, E. Moulin, S. Mueller, R. Mukherjee, P. Munar, M. Munari, C. Mundell, J. Mundet, H. Muraishi, K. Murase, A. Muronga, A. Murphy, N. Nagar, S. Nagataki, T. Nagayoshi, B. K. Nagesh, T. Naito, D. Nakajima, D. Nakajima, T. Nakamori, K. Nakayama, J. Nanni, D. Naumann, P. Nayman, L. Nellen, R. Nemmen, A. Neronov, N. Neyroud, T. Nguyen, T. T. Nguyen, T. Nguyen Trung, L. Nicastro, J. Nicolau-Kukliński, F. Niederwanger, A. Niedźwiecki, J. Niemiec, D. Nieto, M. Nievas-Rosillo, A. Nikolaidis, M. Nikołajuk, K. Nishijima, K. -I. Nishikawa, G. Nishiyama, K. Noda, K. Noda, L. Nogues, S. Nolan, R. Northrop, D. Nosek, M. Nöthe, B. Novosyadlyj, L. Nozka, F. Nunio, L. Oakes, P. O'Brien, C. Ocampo, G. Occhipinti, J. P. Ochoa, A. OFaolain de Bhroithe, R. Oger, Y. Ohira, M. Ohishi, S. Ohm, H. Ohoka, N. Okazaki, A. Okumura, J. -F. Olive, D. Olszowski, R. A. Ong, S. Ono, M. Orienti, R. Orito, A. Orlati, J. Osborne, M. Ostrowski, D. Ottaway, N. Otte, S. Öttl, E. Ovcharov, I. Oya, A. Ozieblo, M. Padovani, I. Pagano, S. Paiano, A. Paizis, J. Palacio, M. Palatka, J. Pallotta, K. Panagiotidis, J. -L. Panazol, D. Paneque, M. Panter, M. R. Panzera, R. Paoletti, M. Paolillo, A. Papayannis, G. Papyan, A. Paravac, J. M. Paredes, G. Pareschi, N. Park, D. Parsons, P. Paśko, S. Pavy, M. Pech, A. Peck, G. Pedaletti, A. Pe'er, S. Peet, D. Pelat, A. Pepato, M. d. C. Perez, L. Perri, M. Perri, M. Persic, M. Persic, A. Petrashyk, P. -O. Petrucci, O. Petruk, B. Peyaud, M. Pfeifer, G. Pfeiffer, G. Piano, D. Pieloth, E. Pierre, F. Pinto de Pinho, C. Pio García, Y. Piret, A. Pisarski, S. Pita, Ł. Platos, R. Platzer, S. Podkladkin, L. Pogosyan, M. Pohl, P. Poinsignon, A. Pollo, A. Porcelli, J. Porthault, W. Potter, S. Poulios, J. Poutanen, E. Prandini, E. Prandini, J. Prast, K. Pressard, G. Principe, F. Profeti, D. Prokhorov, H. Prokoph, M. Prouza, R. Pruchniewicz, G. Pruteanu, E. Pueschel, G. Pühlhofer, I. Puljak, M. Punch, S. Pürckhauer, R. Pyzioł, F. Queiroz, E. J. Quel, J. Quinn, A. Quirrenbach, I. Rafighi, S. Rainò, P. J. Rajda, M. Rameez, R. Rando, R. C. Rannot, M. Rataj, T. Ravel, S. Razzaque, P. Reardon, I. Reichardt, O. Reimann, A. Reimer, O. Reimer, A. Reisenegger, M. Renaud, S. Renner, T. Reposeur, B. Reville, A. Rezaeian, W. Rhode, D. Ribeiro, R. Ribeiro Prado, M. Ribó, G. Richards, M. G. Richer, T. Richtler, J. Rico, J. Ridky, F. Rieger, M. Riquelme, P. R. Ristori, S. Rivoire, V. Rizi, E. Roache, J. Rodriguez, G. Rodriguez Fernandez, J. J. Rodríguez Vázquez, G. Rojas, P. Romano, G. Romeo, M. Roncadelli, J. Rosado, J. Rose, S. Rosen, S. Rosier Lees, D. Ross, G. Rouaix, J. Rousselle, A. C. Rovero, G. Rowell, F. Roy, S. Royer, A. Rubini, B. Rudak, A. Rugliancich, W. Rujopakarn, C. Rulten, M. Rupiński, F. Russo, F. Russo, K. Rutkowski, O. Saavedra, S. Sabatini, B. Sacco, I. Sadeh, E. O. Saemann, S. Safi-Harb, A. Saggion, V. Sahakian, T. Saito, N. Sakaki, S. Sakurai, A. Salamon, M. Salega, D. Salek, F. Salesa Greus, J. Salgado, G. Salina, L. Salinas, A. Salini, D. Sanchez, M. Sanchez-Conde, H. Sandaker, A. Sandoval, P. Sangiorgi, M. Sanguillon, H. Sano, M. Santander, A. Santangelo, E. M. Santos, R. Santos-Lima, A. Sanuy, L. Sapozhnikov, S. Sarkar, K. Satalecka, K. Satalecka, Y. Sato, R. Savalle, M. Sawada, F. Sayède, S. Schanne, T. Schanz, E. J. Schioppa, S. Schlenstedt, J. Schmid, T. Schmidt, J. Schmoll, M. Schneider, H. Schoorlemmer, P. Schovanek, A. Schubert, E. -M. Schullian, J. Schultze, A. Schulz, S. Schulz, K. Schure, F. Schussler, T. Schwab, U. Schwanke, J. Schwarz, T. Schweizer, S. Schwemmer, U. Schwendicke, C. Schwerdt, E. Sciacca, S. Scuderi, A. Segreto, J. -H. Seiradakis, G. H. Sembroski, D. Semikoz, O. Sergijenko, N. Serre, M. Servillat, K. Seweryn, N. Shafi, A. Shalchi, M. Sharma, M. Shayduk, R. C. Shellard, T. Shibata, A. Shigenaka, I. Shilon, E. Shum, L. Sidoli, M. Sidz, J. Sieiro, H. Siejkowski, J. Silk, A. Sillanpää, D. Simone, H. Simpson, B. B. Singh, A. Sinha, G. Sironi, J. Sitarek, P. Sizun, V. Sliusar, V. Sliusar, A. Smith, D. Sobczyńska, H. Sol, G. Sottile, M. Sowiński, F. Spanier, G. Spengler, R. Spiga, R. Stadler, O. Stahl, A. Stamerra, S. Stanič, R. Starling, D. Staszak, Ł. Stawarz, R. Steenkamp, S. Stefanik, C. Stegmann, S. Steiner, C. Stella, M. Stephan, N. Stergioulas, R. Sternberger, M. Sterzel, B. Stevenson, F. Stinzing, M. Stodulska, M. Stodulski, T. Stolarczyk, G. Stratta, U. Straumann, L. Stringhetti, M. Strzys, R. Stuik, K. -H. Sulanke, T. Suomijärvi, A. D. Supanitsky, T. Suric, I. Sushch, P. Sutcliffe, J. Sykes, M. Szanecki, T. Szepieniec, P. Szwarnog, A. Tacchini, K. Tachihara, G. Tagliaferri, H. Tajima, H. Takahashi, K. Takahashi, M. Takahashi, L. Takalo, S. Takami, J. Takata, J. Takeda, G. Talbot, T. Tam, M. Tanaka, S. Tanaka, T. Tanaka, Y. Tanaka, C. Tanci, S. Tanigawa, M. Tavani, F. Tavecchio, J. -P. Tavernet, K. Tayabaly, A. Taylor, L. A. Tejedor, I. Telezhinsky, F. Temme, P. Temnikov, C. Tenzer, Y. Terada, J. C. Terrazas, R. Terrier, D. Terront, T. Terzic, D. Tescaro, M. Teshima, M. Teshima, V. Testa, D. Tezier, J. Thayer, J. Thornhill, S. Thoudam, D. Thuermann, L. Tibaldo, A. Tiengo, M. C. Timpanaro, D. Tiziani, M. Tluczykont, C. J. Todero Peixoto, F. Tokanai, M. Tokarz, K. Toma, J. Tomastik, Y. Tomono, A. Tonachini, D. Tonev, K. Torii, M. Tornikoski, D. F. Torres, M. Torres, E. Torresi, G. Toso, G. Tosti, T. Totani, N. Tothill, F. Toussenel, G. Tovmassian, T. Toyama, P. Travnicek, C. Trichard, M. Trifoglio, I. Troyano Pujadas, M. Trzeciak, K. Tsinganos, S. Tsujimoto, T. Tsuru, Y. Uchiyama, G. Umana, Y. Umetsu, S. S. Upadhya, M. Uslenghi, V. Vagelli, F. Vagnetti, J. Valdes-Galicia, M. Valentino, P. Vallania, L. Valore, W. van Driel, C. van Eldik, B. van Soelen, J. Vandenbroucke, J. Vanderwalt, G. Vasileiadis, V. Vassiliev, J. R. Vázquez, M. L. Vázquez Acosta, M. Vecchi, A. Vega, I. Vegas, P. Veitch, P. Venault, L. Venema, C. Venter, S. Vercellone, S. Vergani, K. Verma, V. Verzi, G. P. Vettolani, C. Veyssiere, A. Viana, N. Viaux, J. Vicha, C. Vigorito, P. Vincent, S. Vincent, J. Vink, V. Vittorini, N. Vlahakis, L. Vlahos, H. Voelk, V. Voisin, A. Vollhardt, A. Volpicelli, H. von Brand, S. Vorobiov, I. Vovk, M. Vrastil, L. V. Vu, T. Vuillaume, R. Wagner, R. Wagner, S. J. Wagner, S. P. Wakely, T. Walstra, R. Walter, T. Walther, J. E. Ward, M. Ward, K. Warda, D. Warren, S. Wassberg, J. J. Watson, P. Wawer, R. Wawrzaszek, N. Webb, P. Wegner, O. Weiner, A. Weinstein, R. Wells, F. Werner, H. Wetteskind, M. White, R. White, M. Więcek, A. Wierzcholska, S. Wiesand, R. Wijers, P. Wilcox, N. Wild, A. Wilhelm, M. Wilkinson, M. Will, M. Will, D. A. Williams, J. T. Williams, R. Willingale, N. Wilson, M. Winde, K. Winiarski, H. Winkler, M. Winter, R. Wischnewski, E. Witt, P. Wojcik, D. Wolf, M. Wood, A. Wörnlein, E. Wu, T. Wu, K. K. Yadav, H. Yamamoto, T. Yamamoto, N. Yamane, R. Yamazaki, S. Yanagita, L. Yang, D. Yelos, A. Yoshida, M. Yoshida, T. Yoshida, S. Yoshiike, T. Yoshikoshi, P. Yu, V. Zabalza, D. Zaborov, M. Zacharias, G. Zaharijas, A. Zajczyk, L. Zampieri, F. Zandanel, R. Zanmar Sanchez, D. Zaric, D. Zavrtanik, M. Zavrtanik, A. Zdziarski, A. Zech, H. Zechlin, A. Zhao, V. Zhdanov, A. Ziegler, J. Ziemann, K. Ziętara, A. Zink, J. Ziółkowski, V. Zitelli, A. Zoli, J. Zorn, P. Żychowski

List of contributions from the Cherenkov Telescope Array (CTA) Consortium presented at the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016), July 11-15, 2016, in Heidelberg, Germany. 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

We report on C-band (5 - 7 GHz) observations of the galaxy, NGC~2992, from the CHANG-ES sample. This galaxy displays an embedded nuclear double-lobed radio morphology within its spiral disk, as revealed in linearly polarized emission but {\it not} in total intensity emission. The radio lobes are kpc-sized, similar to what has been observed in the past for other Seyfert galaxies, and show ordered magnetic fields. Read More

The detailed investigation of the Higgs sector at present and future colliders necessitates from the theory side as precise predictions as possible, including higher order corrections. An important ingredient for the computation of higher order corrections is the renormalization of the model parameters and fields. In this paper we complete the renormalization of the 2-Higgs-Doublet Model (2HDM) Higgs sector launched in a previous contribution with the investigation of the renormalization of the mixing angles $\alpha$ and $\beta$. Read More

The binary millisecond radio pulsar PSR J1023+0038 exhibits many characteristics similar to the gamma-ray binary system PSR B1259--63/LS 2883, making it an ideal candidate for the study of high-energy non-thermal emission. It has been the subject of multi-wavelength campaigns following the disappearance of the pulsed radio emission in 2013 June, which revealed the appearance of an accretion disk around the neutron star. We present the results of very high-energy gamma-ray observations carried out by VERITAS before and after this change of state. Read More

Transient X-ray binaries produce major outbursts in which the X-ray flux can increase over the quiescent level by factors as large as $10^7$. The low-mass X-ray binary V 404 Cyg and the high-mass system 4U 0115+634 underwent such major outbursts in June and October 2015, respectively. We present here observations at energies above hundreds of GeV with the VERITAS observatory taken during some of the brightest X-ray activity ever observed from these systems. Read More

2016Aug

The very high energy (VHE; E $>$ 100 GeV) blazar Markarian 501 was observed between April 17 and May 5 (MJD 54938--54956), 2009, as part of an extensive multi-wavelength campaign from radio to VHE. Strong VHE $\gamma$-ray activity was detected on May 1st with Whipple and VERITAS, when the flux (E $>$ 400 GeV) increased to 10 times the pre-flare baseline flux ($3.9{\times 10^{-11}}~{\rm ph~cm^{-2}~s^{-1}}$), reaching five times the flux of the Crab Nebula. Read More

The positron annihilation gamma-ray signal in the Milky Way (MW) shows a puzzling morphology: a very bright bulge and a very low surface-brightness disk. A coherent explanation of the positron origin, propagation through the Galaxy and subsequent annihilation in the interstellar medium has not yet been found. Tentative explanations involve positrons from radioactivity, X-ray binaries, and dark matter (DM). Read More

We present results from two suites of simulations of powerful radio galaxies in poor cluster environments, with a focus on the formation and evolution of the radio lobes. One suite of models uses relativistic hydrodynamics and the other relativistic magnetohydrodynamics; both are set up to cover a range of jet powers and velocities. The dynamics of the lobes are shown to be in good agreement with analytical models and with previous numerical models, confirming in the relativistic regime that the observed widths of radio lobes may be explained if they are driven by very light jets. Read More

The 2-Higgs-Doublet Model (2HDM) belongs to the simplest extensions of the Standard Model (SM) Higgs sector that are in accordance with theoretical and experimental constraints. In order to be able to properly investigate the experimental Higgs data and, in the long term to distinguish between possible models beyond the SM, precise predictions for the Higgs boson observables have to be made available on the theory side. This requires the inclusion of the higher order corrections. Read More

We investigate the effects of ram pressure on the ordered magnetic field of a galaxy hosting a radio halo and strong nuclear outflows. New radio images in total and polarized intensity of the edge-on Virgo galaxy NGC\,4388 were obtained within the CHANG-ES EVLA project. The unprecedented noise level reached allows us to detect striking new features of the ordered magnetic field. Read More

We describe a method for spectral cleaning and timing calibration of short voltage time series data from individual radio interferometer receivers. It makes use of the phase differences in Fast Fourier Transform (FFT) spectra across antenna pairs. For strong, localized terrestrial sources these are stable over time, while being approximately uniform-random for a sum over many sources or for noise. Read More

We present results from multiwavelength observations of the BL Lacertae object 1ES 1741+196, including results in the very-high-energy $\gamma$-ray regime using the Very Energetic Radiation Imaging Telescope Array System (VERITAS). The VERITAS time-averaged spectrum, measured above 180 GeV, is well-modelled by a power law with a spectral index of $2.7\pm0. Read More

Two-thirds of long duration gamma-ray bursts (GRBs) show soft X-ray absorption in excess of the Milky Way. The column densities of metals inferred from UV and optical spectra differ from those derived from soft X-ray spectra, at times by an order of magnitude, with the latter being higher. The origin of the soft X-ray absorption excess observed in GRB X-ray afterglow spectra remains a heavily debated issue, which has resulted in numerous investigations on the effect of hot material both internal and external to the GRB host galaxy on our X-ray afterglow observations. Read More

Between the beginning of its full-scale scientific operations in 2007 and 2012, the VERITAS Cherenkov telescope array observed more than 130 blazars; of these, 26 were detected as very-high-energy (VHE; E>100 GeV) {\gamma}-ray sources. In this work, we present the analysis results of a sample of 114 undetected objects. The observations constitute a total live-time of ~570 hours. Read More

2016Mar
Authors: M. Arenz, M. Babutzka, M. Bahr, J. P. Barrett, S. Bauer, M. Beck, A. Beglarian, J. Behrens, T. Bergmann, U. Besserer, J. Blümer, L. I. Bodine, K. Bokeloh, J. Bonn, B. Bornschein, L. Bornschein, S. Büsch, T. H. Burritt, S. Chilingaryan, T. J. Corona, L. De Viveiros, P. J. Doe, O. Dragoun, G. Drexlin, S. Dyba, S. Ebenhöch, K. Eitel, E. Ellinger, S. Enomoto, M. Erhard, D. Eversheim, M. Fedkevych, A. Felden, S. Fischer, J. A. Formaggio, F. Fränkle, D. Furse, M. Ghilea, W. Gil, F. Glück, A. Gonzalez Urena, S. Görhardt, S. Groh, S. Grohmann, R. Grössle, R. Gumbsheimer, M. Hackenjos, V. Hannen, F. Harms, N. Hauÿmann, F. Heizmann, K. Helbing, W. Herz, S. Hickford, D. Hilk, B. Hillen, T. Höhn, B. Holzapfel, M. Hötzel, M. A. Howe, A. Huber, A. Jansen, N. Kernert, L. Kippenbrock, M. Kleesiek, M. Klein, A. Kopmann, A. Kosmider, A. Kovalík, B. Krasch, M. Kraus, H. Krause, M. Krause, L. Kuckert, B. Kuffner, L. La Cascio, O. Lebeda, B. Leiber, J. Letnev, V. M. Lobashev, A. Lokhov, E. Malcherek, M. Mark, E. L. Martin, S. Mertens, S. Mirz, B. Monreal, K. Müller, M. Neuberger, H. Neumann, S. Niemes, M. Noe, N. S. Oblath, A. Off, H. -W. Ortjohann, A. Osipowicz, E. Otten, D. S. Parno, P. Plischke, A. W. P. Poon, M. Prall, F. Priester, P. C. -O. Ranitzsch, J. Reich, O. Rest, R. G. H. Robertson, M. Röllig, S. Rosendahl, S. Rupp, M. Rysavy, K. Schlösser, M. Schlösser, K. Schönung, M. Schrank, J. Schwarz, W. Seiler, H. Seitz-Moskaliuk, J. Sentkerestiova, A. Skasyrskaya, M. Slezak, A. Spalek, M. Steidl, N. Steinbrink, M. Sturm, M. Suesser, H. H. Telle, T. Thümmler, N. Titov, I. Tkachev, N. Trost, A. Unru, K. Valerius, D. Venos, R. Vianden, S. Vöcking, B. L. Wall, N. Wandkowsky, M. Weber, C. Weinheimer, C. Weiss, S. Welte, J. Wendel, K. L. Wierman, J. F. Wilkerson, D. Winzen, J. Wolf, S. Wüstling, M. Zacher, S. Zadoroghny, M. Zboril

The KATRIN experiment will probe the neutrino mass by measuring the beta-electron energy spectrum near the endpoint of tritium beta-decay. An integral energy analysis will be performed by an electro-static spectrometer (Main Spectrometer), an ultra-high vacuum vessel with a length of 23.2 m, a volume of 1240 m^3, and a complex inner electrode system with about 120000 individual parts. Read More

Microquasars are stellar-mass black holes accreting matter from a companion star and ejecting plasma jets at almost the speed of light. They are analogues of quasars that contain supermassive black holes of $10^6$ to $10^{10}$ solar masses. Accretion in microquasars varies on much shorter timescales than in quasars and occasionally produces exceptionally bright X-ray flares. Read More

We present 1D cosmic ray transport models, numerically solving equations of pure advection and diffusion for the electrons and calculating synchrotron emission spectra. We find that for exponential halo magnetic field distributions advection leads to approximately exponential radio continuum intensity profiles, whereas diffusion leads to profiles that can be better approximated by a Gaussian function. Accordingly, the vertical radio spectral profiles for advection are approximately linear, whereas for diffusion they are of `parabolic' shape. Read More

The F-type star KIC 8462852 has recently been identified as an exceptional target for SETI (search for extraterrestrial intelligence) observations. We describe an analysis methodology for optical SETI, which we have used to analyse nine hours of serendipitous archival observations of KIC 8462852 made with the VERITAS gamma-ray observatory between 2009 and 2015. No evidence of pulsed optical beacons, above a pulse intensity at the Earth of approximately 1 photon per m^2, is found. Read More

The TeV binary system LS I +61$^\circ$ 303 is known for its regular, non-thermal emission pattern which traces the orbital period of the compact object in its 26.5 day orbit around its B0 Ve star companion. The system typically presents elevated TeV emission around apastron passage with flux levels between 5% and 15% of the steady flux from the Crab Nebula (> 300 GeV). Read More

Gas expulsion is a central concept in some of the models for multiple populations and the light-element anticorrelations in globular clusters. If the star formation efficiency was around 30 per cent and the gas expulsion happened on the crossing timescale, this process could expel preferentially stars born with the chemical composition of the proto-cluster gas, while stars with special composition born in the centre would remain bound. Recently, a sample of extragalactic, gas-free, young massive clusters has been identified that has the potential to test the conditions for gas expulsion. Read More

2015Dec
Authors: A. U. Abeysekara1, S. Archambault2, A. Archer3, T. Aune4, A. Barnacka5, W. Benbow6, R. Bird7, J. Biteau8, J. H. Buckley9, V. Bugaev10, J. V Cardenzana11, M. Cerruti12, X. Chen13, J. L. Christiansen14, L. Ciupik15, M. P. Connolly16, P. Coppi17, W. Cui18, H. J. Dickinson19, J. Dumm20, J. D. Eisch21, M. Errando22, A. Falcone23, Q. Feng24, J. P. Finley25, H. Fleischhack26, A. Flinders27, P. Fortin28, L. Fortson29, A. Furniss30, G. H. Gillanders31, S. Griffin32, J. Grube33, G. Gyuk34, M. Hütten35, N. Håkansson36, D. Hanna37, J. Holder38, T. B. Humensky39, C. A. Johnson40, P. Kaaret41, P. Kar42, N. Kelley-Hoskins43, Y. Khassen44, D. Kieda45, M. Krause46, F. Krennrich47, S. Kumar48, M. J. Lang49, G. Maier50, S. McArthur51, A. McCann52, K. Meagher53, P. Moriarty54, R. Mukherjee55, D. Nieto56, A. O'Faoláin de Bhróithe57, R. A. Ong58, A. N. Otte59, N. Park60, J. S. Perkins61, A. Petrashyk62, M. Pohl63, A. Popkow64, E. Pueschel65, J. Quinn66, K. Ragan67, G. Ratliff68, P. T. Reynolds69, G. T. Richards70, E. Roache71, J. Rousselle72, M. Santander73, G. H. Sembroski74, K. Shahinyan75, A. W. Smith76, D. Staszak77, I. Telezhinsky78, N. W. Todd79, J. V. Tucci80, J. Tyler81, V. V. Vassiliev82, S. Vincent83, S. P. Wakely84, O. M. Weiner85, A. Weinstein86, A. Wilhelm87, D. A. Williams88, B. Zitzer89, P. S. Smith90, T. W. -S. Holoien91, J. L. Prieto92, C. S. Kochanek93, K. Z. Stanek94, B. Shappee95, T. Hovatta96, W. Max-Moerbeck97, T. J. Pearson98, R. A. Reeves99, J. L. Richards100, A. C. S. Readhead101, G. M. Madejski102, S. G. Djorgovski103, A. J. Drake104, M. J. Graham105, A. Mahabal106
Affiliations: 1VERITAS, 2VERITAS, 3VERITAS, 4VERITAS, 5VERITAS, 6VERITAS, 7VERITAS, 8VERITAS, 9VERITAS, 10VERITAS, 11VERITAS, 12VERITAS, 13VERITAS, 14VERITAS, 15VERITAS, 16VERITAS, 17VERITAS, 18VERITAS, 19VERITAS, 20VERITAS, 21VERITAS, 22VERITAS, 23VERITAS, 24VERITAS, 25VERITAS, 26VERITAS, 27VERITAS, 28VERITAS, 29VERITAS, 30VERITAS, 31VERITAS, 32VERITAS, 33VERITAS, 34VERITAS, 35VERITAS, 36VERITAS, 37VERITAS, 38VERITAS, 39VERITAS, 40VERITAS, 41VERITAS, 42VERITAS, 43VERITAS, 44VERITAS, 45VERITAS, 46VERITAS, 47VERITAS, 48VERITAS, 49VERITAS, 50VERITAS, 51VERITAS, 52VERITAS, 53VERITAS, 54VERITAS, 55VERITAS, 56VERITAS, 57VERITAS, 58VERITAS, 59VERITAS, 60VERITAS, 61VERITAS, 62VERITAS, 63VERITAS, 64VERITAS, 65VERITAS, 66VERITAS, 67VERITAS, 68VERITAS, 69VERITAS, 70VERITAS, 71VERITAS, 72VERITAS, 73VERITAS, 74VERITAS, 75VERITAS, 76VERITAS, 77VERITAS, 78VERITAS, 79VERITAS, 80VERITAS, 81VERITAS, 82VERITAS, 83VERITAS, 84VERITAS, 85VERITAS, 86VERITAS, 87VERITAS, 88VERITAS, 89VERITAS, 90SPOL, 91ASAS-SN, 92ASAS-SN, 93ASAS-SN, 94ASAS-SN, 95ASAS-SN, 96OVRO, 97OVRO, 98OVRO, 99OVRO, 100OVRO, 101OVRO, 102NuSTAR, 103CRTS, 104CRTS, 105CRTS, 106CRTS

Outbursts from gamma-ray quasars provide insights on the relativistic jets of active galactic nuclei and constraints on the diffuse radiation fields that fill the Universe. The detection of significant emission above 100 GeV from a distant quasar would show that some of the radiated gamma rays escape pair-production interactions with low-energy photons, be it the extragalactic background light (EBL), or the radiation near the supermassive black hole lying at the jet's base. VERITAS detected gamma-ray emission up to 200 GeV from PKS 1441+25 (z=0. Read More

2015Dec
Authors: M. Baloković, D. Paneque, G. Madejski, A. Furniss, J. Chiang, the NuSTAR team, :, M. Ajello, D. M. Alexander, D. Barret, R. Blandford, S. E. Boggs, F. E. Christensen, W. W. Craig, K. Forster, P. Giommi, B. W. Grefenstette, C. J. Hailey, F. A. Harrison, A. Hornstrup, T. Kitaguchi, J. E. Koglin, K. K. Madsen, P. H. Mao, H. Miyasaka, K. Mori, M. Perri, M. J. Pivovaroff, S. Puccetti, V. Rana, D. Stern, G. Tagliaferri, C. M. Urry, N. J. Westergaard, W. W. Zhang, A. Zoglauer, the VERITAS collaboration, :, S. Archambault, A. A. Archer, A. Barnacka, W. Benbow, R. Bird, J. Buckley, V. Bugaev, M. Cerruti, X. Chen, L. Ciupik, M. P. Connolly, W. Cui, H. J. Dickinson, J. Dumm, J. D. Eisch, A. Falcone, Q. Feng, J. P. Finley, H. Fleischhack, L. Fortson, S. Griffin, S. T. Griffiths, J. Grube, G. Gyuk, M. Huetten, N. Haakansson, J. Holder, T. B. Humensky, C. A. Johnson, P. Kaaret, M. Kertzman, Y. Khassen, D. Kieda, M. Krause, F. Krennrich, M. J. Lang, G. Maier, S. McArthur, K. Meagher, P. Moriarty, T. Nelson, D. Nieto, R. A. Ong, N. Park, M. Pohl, A. Popkow, E. Pueschel, P. T. Reynolds, G. T. Richards, E. Roache, M. Santander, G. H. Sembroski, K. Shahinyan, A. W. Smith, D. Staszak, I. Telezhinsky, N. W. Todd, J. V. Tucci, J. Tyler, S. Vincent, A. Weinstein, A. Wilhelm, D. A. Williams, B. Zitzer, the MAGIC collaboration, :, M. L. Ahnen, S. Ansoldi, L. A. Antonelli, P. Antoranz, A. Babic, B. Banerjee, P. Bangale, U. Barres de Almeida, J. Barrio, J. Becerra González, W. Bednarek, E. Bernardini, B. Biasuzzi, A. Biland, O. Blanch, S. Bonnefoy, G. Bonnoli, F. Borracci, T. Bretz, E. Carmona, 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. D. de Oña Wilhelmi, C. Delgado Mendez, F. Di Pierro, D. Dominis Prester, D. Dorner, M. Doro, S. Einecke, D. Elsaesser, 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, D. Eisenacher, N. Godinović, A. González Muñoz, D. Guberman, 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. López, R. López-Coto, A. López-Oramas, E. Lorenz, 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, R. Orito, A. Overkemping, S. Paiano, S. Palacio, M. Palatiello, R. Paoletti, J. M. Paredes, X. Paredes-Fortuny, M. Persic, J. Poutanen, P. G. Prada Moroni, E. Prandini, I. Puljak, W. Rhode, M. Ribó, J. Rico, J. Rodriguez Garcia, T. Saito, K. Satalecka, V. Scapin, C. Schultz, T. Schweizer, S. N. Shore, A. Sillanpää, J. Sitarek, I. Snidaric, D. Sobczynska, A. Stamerra, T. Steinbring, M. Strzys, L. O. Takalo, H. Takami, F. Tavecchio, P. Temnikov, T. Terzić, D. Tescaro, M. Teshima, J. Thaele, D. F. Torres, T. Toyama, A. Treves, V. Verguilov, I. Vovk, J. E. Ward, M. Will, M. H. Wu, R. Zanin, external collaborators, :, J. Perkins, F. Verrecchia, C. Leto, M. Böttcher, M. Villata, C. M. Raiteri, J. A. Acosta-Pulido, R. Bachev, A. Berdyugin, D. A. Blinov, M. I. Carnerero, W. P. Chen, P. Chinchilla, G. Damljanovic, C. Eswaraiah, T. S. Grishina, S. Ibryamov, B. Jordan, S. G. Jorstad, M. Joshi, E. N. Kopatskaya, O. M. Kurtanidze, S. O. Kurtanidze, E. G. Larionova, L. V. Larionova, V. M. Larionov, G. Latev, H. C. Lin, A. P. Marscher, A. A. Mokrushina, D. A. Morozova, M. G. Nikolashvili, E. Semkov, A. Strigachev, Yu. V. Troitskaya, I. S. Troitsky, O. Vince, J. Barnes, T. Güver, J. W. Moody, A. C. Sadun, S. Sun, T. Hovatta, J. L. Richards, W. Max-Moerbeck, A. C. Readhead, A. Lähteenmäki, M. Tornikoski, J. Tammi, V. Ramakrishnan, R. Reinthal, E. Angelakis, L. Fuhrmann, I. Myserlis, V. Karamanavis, A. Sievers, H. Ungerechts, J. A. Zensus

We present coordinated multiwavelength observations of the bright, nearby BL Lac object Mrk 421 taken in 2013 January-March, involving GASP-WEBT, Swift, NuSTAR, Fermi-LAT, MAGIC, VERITAS, and other collaborations and instruments, providing data from radio to very-high-energy (VHE) gamma-ray bands. NuSTAR yielded previously unattainable sensitivity in the 3-79 keV range, revealing that the spectrum softens when the source is dimmer until the X-ray spectral shape saturates into a steep power law with a photon index of approximately 3, with no evidence for an exponential cutoff or additional hard components up to about 80 keV. For the first time, we observed both the synchrotron and the inverse-Compton peaks of the spectral energy distribution (SED) simultaneously shifted to frequencies below the typical quiescent state by an order of magnitude. Read More

The annihilation of positrons in the Galaxy's interstellar medium produces characteristic gamma-rays with a line at 511 keV. This emission has been observed with the spectrometer SPI on INTEGRAL, confirming a puzzling morphology with bright emission from an extended bulge-like region, and faint disk emission. Most plausible sources of positrons are believed to be distributed throughout the disk of the Galaxy. Read More

How a galaxy regulates its SNe energy into different interstellar/circumgalactic medium components strongly affects galaxy evolution. Based on the JVLA D-configuration C- (6 GHz) and L-band (1.6 GHz) continuum observations, we perform statistical analysis comparing multi-wavelength properties of the CHANG-ES galaxies. Read More

Stellar winds and supernova (SN) explosions of massive stars ("stellar feedback") create bubbles in the interstellar medium (ISM) and insert newly produced heavy elements and kinetic energy into their surroundings, possibly driving turbulence. Most of this energy is thermalized and immediately removed from the ISM by radiative cooling. The rest is available for driving ISM dynamics. Read More

Compilation of papers presented by the VERITAS Collaboration at the 34th International Cosmic Ray Conference (ICRC), held July 30 through August 6, 2015 in The Hague, The Netherlands. Read More

The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is a ground-based array located at the Fred Lawrence Whipple Observatory in southern Arizona and is one of the world's most sensitive gamma-ray instruments at energies of 85 GeV to $>$30 TeV. VERITAS has a wide scientific reach that includes the study of extragalactic and Galactic objects as well as the search for astrophysical signatures of dark matter and the measurement of cosmic rays. In this paper, we will summarize the current status of the VERITAS observatory and present some of the scientific highlights from the last two years, focusing in particular on those results shown at the 2015 ICRC in The Hague, Netherlands. Read More

The Lupus I cloud is found between the Upper-Scorpius (USco) and the Upper-Centaurus-Lupus (UCL) sub-groups of the Sco-Cen OB-association, where the expanding USco H I shell appears to interact with a bubble currently driven by the winds of the remaining B-stars of UCL.We want to study how collisions of large-scale interstellar gas flows form and influence new dense clouds in the ISM.We performed LABOCA continuum sub-mm observations of Lupus I that provide for the first time a direct view of the densest, coldest cloud clumps and cores at high angular resolution. Read More

2015Sep
Authors: A. Furniss1, K. Noda2, S. Boggs3, J. Chiang4, F. Christensen5, W. Craig6, P . Giommi7, C. Hailey8, F. Harisson9, G. Madejski10, K. Nalewajko11, M. Perri12, D. Stern13, M. Urry14, F. Verrecchia15, W. Zhang16, M. L. Ahnen17, S. Ansoldi18, L. A. Antonelli19, P. Antoranz20, A. Babic21, B. Banerjee22, P. Bangale23, U. Barres de Almeida24, J. A. Barrio25, J. Becerra Gonzalez26, W. Bednarek27, E. Bernardini28, B. Biasuzzi29, A. Biland30, O. Blanch31, S. Bonnefoy32, G. Bonnoli33, F. Borracci34, T. Bretz35, E. Carmona36, A. Carosi37, A. Chatterjee38, R. Clavero39, P. Colin40, E. Colombo41, J. L. Contreras42, J. Cortina43, S. Covino44, P. Da Vela45, F. Dazzi46, A. De Angelis47, G. De Caneva48, B. De Lotto49, E. de Ona Wilhelmi50, C. Delgado Mendez51, F. Di Pierro52, D. Dominis Prester53, D. Dorner54, M. Doro55, S. Einecke56, D. Eisenacher Glawion57, D. Elsaesser58, A. Fernandez-Barral59, D. Fidalgo60, M. V. Fonseca61, L. Font62, K. Frantzen63, C. Fruck64, D. Galindo65, R. J. Garcia Lopez66, M. Garczarczyk67, D. Garrido Terrats68, M. Gaug69, P. Giammaria70, N. Godinovic71, A. Gonzalez Munoz72, D. Guberman73, Y. Hanabata74, M. Hayashida75, J. Herrera76, J. Hose77, D. Hrupec78, G. Hughes79, W. Idec80, H. Kellermann81, K. Kodani82, Y. Konno83, H. Kubo84, J. Kushida85, A. La Barbera86, D. Lelas87, N. Lewandowska88, E. Lindfors89, S. Lombardi90, F. Longo91, M. Lopez92, R. Lopez-Coto93, A. Lopez-Oramas94, E. Lorenz95, P. Majumdar96, M. Makariev97, K. Mallot98, G. Maneva99, M. Manganaro100, K. Mannheim101, L. Maraschi102, B. Marcote103, M. Mariotti104, M. Martinez105, D. Mazin106, U. Menzel107, J. M. Miranda108, R. Mirzoyan109, A. Moralejo110, D. Nakajima111, V. Neustroev112, A. Niedzwiecki113, M. Nievas Rosillo114, K. Nilsson115, K. Nishijima116, R. Orito117, A. Overkemping118, S. Paiano119, J. Palacio120, M. Palatiello121, D. Paneque122, R. Paoletti123, J. M. Paredes124, X. Paredes-Fortuny125, M. Persic126, J. Poutanen127, P. G. Prada Moroni128, E. Prandini129, I. Puljak130, R. Reinthal131, W. Rhode132, M. Ribo133, J. Rico134, J. Rodriguez Garcia135, T. Saito136, K. Saito137, K. Satalecka138, V. Scapin139, C. Schultz140, T. Schweizer141, S. N. Shore142, A. Sillanpaa143, J. Sitarek144, I. Snidaric145, D. Sobczynska146, A. Stamerra147, T. Steinbring148, M. Strzys149, L. Takalo150, H. Takami151, F. Tavecchio152, P. Temnikov153, T. Terzic154, D. Tescaro155, M. Teshima156, J. Thaele157, D. F. Torres158, T. Toyama159, A. Treves160, V. Verguilov161, I. Vovk162, M. Will163, R. Zanin164, A. Archer165, W. Benbow166, R. Bird167, J. Biteau168, V. Bugaev169, J. V Cardenzana170, M. Cerruti171, X. Chen172, L. Ciupik173, M. P. Connolly174, W. Cui175, H. J. Dickinson176, J. Dumm177, J. D. Eisch178, A. Falcone179, Q. Feng180, J. P. Finley181, H. Fleischhack182, P. Fortin183, L. Fortson184, L. Gerard185, G. H. Gillanders186, S. Griffin187, S. T. Griffiths188, J. Grube189, G. Gyuk190, N. Haakansson191, J. Holder192, T. B. Humensky193, C. A. Johnson194, P. Kaaret195, M. Kertzman196, D. Kieda197, M. Krause198, F. Krennrich199, M. J. Lang200, T. T. Y. Lin201, G. Maier202, S. McArthur203, A. McCann204, K. Meagher205, P. Moriarty206, R. Mukherjee207, D. Nieto208, A. O'Faolain de Bhroithe209, R. A. Ong210, N. Park211, D. Petry212, M. Pohl213, A. Popkow214, K. Ragan215, G. Ratliff216, L. C. Reyes217, P. T. Reynolds218, G. T. Richards219, E. Roache220, M. Santander221, G. H. Sembroski222, K. Shahinyan223, D. Staszak224, I. Telezhinsky225, J. V. Tucci226, J. Tyler227, V. V. Vassiliev228, S. P. Wakely229, O. M. Weiner230, A. Weinstein231, A. Wilhelm232, D. A. Williams233, B. Zitzer234, O. Vince L. Fuhrmann235, E. Angelakis236, V. Karamanavis237, I. Myserlis238, T. P. Krichbaum239, J. A. Zensus240, H. Ungerechts241, A. Sievers242, R. Bachev, M. Bottcher, W. P. Chen, G. Damljanovic, C. Eswaraiah, T. Guver, T. Hovatta, Z. Hughes, S. . I. Ibryamov, M. D. Joner, B. Jordan, S. G. Jorstad,