Zobrazeno 1 - 10
of 94
pro vyhledávání: '"M. Shayduk"'
Autor:
Vladimir G. Kolmogorov, Ivan V. Molodkin, Vladimir K. Konovalov, Alexander M. Shayduk, Sergey A. Ostanin, Sergey L. Leonov, Olga V. Borisenko, Mikhail A. Fedoseyev, Julia S. Modakalova
Publikováno v:
Бюллетень сибирской медицины, Vol 16, Iss 2, Pp 136-145 (2017)
Background. Visualization of infiltration in lung tissue surrounding the globular formation of the lungs (GFL) determined by X-ray is one of the important points in the differential diagnosis of primary lung cancer, specific and non-specific inflamma
Externí odkaz:
https://doaj.org/article/305e528648ff4e90a6808fb7367a8b9a
Autor:
R. Maier, Takashi Saito, Derek Strom, S. Metz, D. Corti, M. Shayduk, T. Schweizer, R. Mirzoyan, J. R. Garcia, D. Häfner, S. Tran, D. Nakajima, Francesco Dazzi, G. Ceribella, Mosè Mariotti, A. Dettlaff, Martin Will, Masahiro Teshima, D. Herranz, Julian Sitarek, M. Lopez-Moya
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
instname
The current generation of ground-based imaging atmospheric Cherenkov telescopes (IACTs) operate in the very-high-energy (VHE) domain from similar to 100 GeV to similar to 100 TeV. They use electronic digital trigger systems to discern the Cherenkov l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0dc0504887543500ce3ff9f0a7fe635c
Autor:
A. M. Shayduk, S. A. Ostanin
Publikováno v:
Biomedical Engineering. 49:160-163
A device for noninvasive measurement of the repetition frequency of single-motor-unit action potential is described. The device was built using virtual instruments in LabVIEW software. The mathematical foundations of the measurement method and result
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6263ae66d8ed3496c45310959157bc8e
https://doi.org/10.1007/s10527-015-9520-z
https://doi.org/10.1007/s10527-015-9520-z
Publikováno v:
Nuclear instruments & methods in physics research / A 782, 92-103 (2015). doi:10.1016/j.nima.2015.01.096
This paper describes the concept of an FPGA-based digital camera trigger for imaging atmospheric Cherenkov telescopes, developed for the future Cherenkov Telescope Array (CTA). The proposed camera trigger is designed to select images initiated by the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::119bd918a020d00740c330de579fa04d
https://doi.org/10.1016/j.nima.2015.01.096
https://doi.org/10.1016/j.nima.2015.01.096
Autor:
Tomasz Szepieniec, K. Nishijima, T. Grabarczyk, M. C. Maccarone, Thomas Lohse, F. de Palma, Jacek Niemiec, R. J. García López, S. Rainò, Stefan Ohm, G. Busetto, F. Nunio, G. Pareschi, Emmanuel Moulin, Michał Szanecki, Jiri Chudoba, Saverio Lombardi, M. Nievas, Massimo Persic, A. Wilhelm, A. Bonardi, D. Garrido, J. L. Dournaux, A. Förster, Vikram V. Dwarkadas, Juan Abel Barrio, F. Di Pierro, K. Meagher, A. C. Rovero, Paweł Wójcik, Martina Bohacova, A. Sillanpää, Giuseppe Malaguti, R. A. Ong, Jörg R. Hörandel, Włodek Kluźniak, Henrike Fleischhack, Valerie Connaughton, Juhani Huovelin, Dusan Mandat, B. De Lotto, M. Palatka, Francesco Dazzi, A. De Franco, Carla Aramo, Martin Pohl, Anton N. Baushev, H. Siejkowski, G. Lamanna, David Berge, P. Vallania, M. Shayduk, C. van Eldik, N. Giglietto, Alicja Wierzcholska, S. Kaufmann, A. Giuliani, T. B. Humensky, T. Di Girolamo, R. López-Coto, L. Tibaldo, Masatoshi Ohishi, Pratik Majumdar, Luis Ángel Tejedor, B. S. Acharya, B. García, Gernot Maier, D. Nosek, Gagik Tovmassian, J.-P. Lenain, B. Khélifi, Takanori Yoshikoshi, Stanislav Stefanik, P. M. Chadwick, I. de la Calle, Garret Cotter, Masahiro Teshima, M. Fesquet, S. P. Wakely, William H. Lee, Andreas Quirrenbach, U. F. Katz, M. Garczarczyk, P. Romano, P. A. Caraveo, O. Tibolla, Marek Jamrozy, Nikola Godinovic, N. Otte, Hidetoshi Kubo, M. Fuessling, G. Fontaine, Rodolfo Carosi, Tarek M. Hassan, S. Vercellone, R. de los Reyes Lopez, Vito Conforti, Carlo Vigorito, Ll. Font, M. Prouza, V. Bugaev, Petr Travnicek, M. Hrabovsky, Jan Ebr, G. Rodriguez Fernandez, Miroslav Pech, Reiko Orito, J. Kocot, Ana Babić, A. Morselli, A. M. Brown, B. Rudak, M. N. Mazziotta, Kathrin Egberts, F. Lucarelli, Nukri Komin, J. Kushida, Jose Luis Contreras, Ferdinando Giordano, Alicia López-Oramas, J. Carr, Nestor Mirabal, C. Di Giulio, P. Kaaret, Petr Janecek, M. Trzeciak, Stefan Wagner, T. Stolarczyk, M. Gaug, Michael G. Burton, Petr Schovanek, A. Weinstein, Maria Magdalena González, I. Telezhinsky, J. Becker Tjus, F. Gargano, Dario Hrupec, Tomasz Bulik
Publikováno v:
Astroparticle Physics, 62, 0, pp. 152-164
Astroparticle Physics
Astroparticle Physics, 2015, 62, pp.152-164. ⟨10.1016/j.astropartphys.2014.08.005⟩
Astroparticle physics 62, 152-164 (2015). doi:10.1016/j.astropartphys.2014.08.005
Astroparticle Physics, Elsevier, 2015, 62, pp.152-164. ⟨10.1016/j.astropartphys.2014.08.005⟩
Astroparticle Physics, 62, 152-164. Elsevier
Astroparticle Physics, 62, 152-164
Astroparticle physics, 2015, Vol.62, pp.152-164 [Peer Reviewed Journal]
Astroparticle Physics
Astroparticle Physics, 2015, 62, pp.152-164. ⟨10.1016/j.astropartphys.2014.08.005⟩
Astroparticle physics 62, 152-164 (2015). doi:10.1016/j.astropartphys.2014.08.005
Astroparticle Physics, Elsevier, 2015, 62, pp.152-164. ⟨10.1016/j.astropartphys.2014.08.005⟩
Astroparticle Physics, 62, 152-164. Elsevier
Astroparticle Physics, 62, 152-164
Astroparticle physics, 2015, Vol.62, pp.152-164 [Peer Reviewed Journal]
Supernova remnants (SNRs) are among the most important targets for γ-ray observatories. Being prominent non-thermal sources, they are very likely responsible for the acceleration of the bulk of Galactic cosmic rays (CRs). To firmly establish the SNR
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f7631599ec1c1a74d63558522ff5425
https://doi.org/10.1016/j.astropartphys.2014.08.005
https://doi.org/10.1016/j.astropartphys.2014.08.005
Autor:
H. Anderhub, K. Shinozaki, Stefano Ciprini, M. Camara, R. Mirzoyan, E. Carmona, Roberta Zanin, Florian Goebel, M. V. Fonseca, P. Jacon, Jorge Andres Lopez Lopez, D. Hakobyan, F. Zandanel, E. Domingo-Santamaría, J. Hose, Jelena Ninkovic, Michela Fagiolini, Oriana Mansutti, Francesco Dazzi, M. Rissi, S. Mizobuchi, Tadeusz Wibig, V. Scalzotto, M. A. Lopez, T. Schweizer, Francesco Longo, W. Wittek, Marc Ribó, J. Zapatero, D. Tescaro, Pol Bordas, Dorota Sobczyńska, M. T. Costado, V. Vitale, C. C. Hsu, Miriam Lucio Martinez, Justin Albert, M. Asensio, Steven N. Shore, V. Curtef, R. Schmitt, Riccardo Paoletti, Takashi Saito, Masahiro Teshima, Igor Oya, Jose Flix, G. Maneva, Daniel Nieto, Daniel Kranich, C. Merck, E. Aliu, E. Prandini, P. Antoranz, Elina Lindfors, Ll. Font, R. K. Bock, C. Baixeras, A. Sillanpää, A. Herrero, A. Saggion, L. O. Takalo, Adrian Biland, S. Rügamer, C. Delgado, V. Danielyan, Masaaki Hayashida, Antonio Stamerra, Juan Abel Barrio, Diego F. Torres, Ciro Bigongiari, M. Pasanen, R. G. Pegna, Markus Gaug, K. Berger, A. Armada, J. Rico, Jose Luis Contreras, Mosè Mariotti, M. Garczarczyk, Josep M. Paredes, M. Shayduk, T. Jogler, Ashot Chilingarian, Juan Cortina, E. Oña-Wilhelmi, R. Kritzer, A. Raymers, A. De Angelis, R. Firpo, B. De Lotto, D. Höhne, L. S. Stark, R. J. García-López, N. Puchades, A. Piccioli, Nicola Galante, R. Kosyra, Robert Wagner, Saverio Lombardi, H. Bartko, E. Fernandez, E. Lorenz, I. Britvitch, Daniel Ferenc, Maria Giller, Thomas Bretz, H. Vankov, Abelardo Moralejo, Michele Doro, N. Otte, M. Panniello, P. Sartori, D. Mazin, Manel Errando, Kari Nilsson, Wolfgang Rhode, Julia Becker, S. Commichau, Wlodek Bednarek, Jose Miguel Miranda, Daniela Dorner, A. Laille, Petar Temnikov, M. Fuchs, Massimo Persic, Mario Meucci, J. A. Coarasa, Valentí Bosch-Ramon, L. Peruzzo, V. Scapin, R. de los Reyes, Nicola Turini, P. Majumdar, N. Sidro, M. Meyer, D. Pascoli, A. Robert, Felicitas Pauss, T. Hengstebeck, Denis Bastieri, Alvaro Sanchez, Karl Mannheim
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 594:407-419
Until April 2007 the MAGIC telescope used a 300 MSamples/s FADC system to sample the shaped PMT signals produced by the captured Cherenkov photons of air showers. Different algorithms to reconstruct the signal from the read-out samples (extractors) h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8fb3d72f3d2dd1c7733e02cab6235b7e
https://doi.org/10.1016/j.nima.2008.06.043
https://doi.org/10.1016/j.nima.2008.06.043
Autor:
E. Fernandez, M. I. Martínez, K. Shinozaki, V. Danielyan, R. K. Bock, N. Sidro, A. Laille, J. M. Paredes, Antonio Stamerra, Francesco Longo, W. Wittek, D. Pascoli, Roberta Zanin, M. Fuchs, Massimo Persic, F. Pauss, E. Lorenz, T. Hengstebeck, E. Domingo-Santamaría, Michela Fagiolini, Oriana Mansutti, M. Pasanen, Abelardo Moralejo, R. de los Reyes, Stefano Ciprini, D. Hakobyan, S. Mizobuchi, Denis Bastieri, A. Robert, Nicola Turini, Jelena Ninkovic, R. Firpo, Alvaro Sanchez, Marc Ribó, K. Nilsson, M. T. Costado, C. Baixeras, H. Anderhub, Julia Becker, Francesco Dazzi, S. Commichau, J. A. Coarasa, D. Tescaro, Tadeusz Wibig, Dorota Sobczyńska, P. Antoranz, J. Zapatero, Justin Albert, Jose Miguel Miranda, Juan Abel Barrio, V. Vitale, I. Oya, J. Rico, G. Maneva, A. Saggion, F. Zandanel, Daniel Nieto, Adrian Biland, Mario Meucci, E. Carmona, Markus Gaug, N. Otte, C. Merck, C. Delgado, K. Berger, L. Peruzzo, K. Mannheim, E. Aliu, Elina Lindfors, L. S. Stark, M. Meyer, Daniel Mazin, Riccardo Paoletti, Michele Doro, M. V. Fonseca, M. Garczarczyk, S. Rügamer, Elisa Prandini, V. Curtef, M. Camara, Ashot Chilingarian, Maria Giller, M. Shayduk, Diego F. Torres, Ciro Bigongiari, Manel Errando, L. O. Takalo, A. Raymers, Pol Bordas, A. Herrero, Mosè Mariotti, A. De Angelis, A. Piccioli, Nicola Galante, P. Sartori, Saverio Lombardi, R. Kritzer, M. Asensio, B. De Lotto, M. López, R. Schmitt, R. Kosyra, Robert Wagner, H. Bartko, E. Oña-Wilhelmi, N. Puchades, P. Jacon, C. C. Hsu, A. Armada, Thomas Bretz, S. N. Shore, R. Mirzoyan, M. Panniello, Masahiro Teshima, Wolfgang Rhode, T. Schweizer, I. Britvitch, A. Sillanpää, W. Bednarek, Jose Flix, Ll. Font, Takashi Saito, Daniela Dorner, J. Hose, Petar Temnikov, Valentí Bosch-Ramon, V. Scapin, Florian Goebel, Masaaki Hayashida, Jose Luis Contreras, Juan Cortina, R. Pegna, Daniel Ferenc, H. Vankov, P. Majumdar, Jorge Andres Lopez Lopez, V. Scalzotto, M. Rissi, D. Kranich, T. Jogler, D. Höhne, R. J. García-López
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The paper describes the different methods, used in the MAGIC experiment, to unfold experimental energy distributions of cosmic ray particles (gamma-rays). Questions and problems related to the unfolding are discussed. Various procedures are proposed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::706b6fd10aba91f56abb239a9b1c7443
https://doi.org/10.1016/j.nima.2007.09.048
https://doi.org/10.1016/j.nima.2007.09.048
Autor:
J. Albert, E. Aliu, H. Anderhub, P. Antoranz, A. Armada, C. Baixeras, J. A. Barrio, H. Bartko, D. Bastieri, J. K. Becker, W. Bednarek, K. Berger, C. Bigongiari, A. Biland, R. K. Bock, P. Bordas, V. Bosch‐Ramon, T. Bretz, I. Britvitch, M. Camara, E. Carmona, A. Chilingarian, J. A. Coarasa, S. Commichau, J. L. Contreras, J. Cortina, M. T. Costado, V. Curtef, V. Danielyan, F. Dazzi, A. De Angelis, C. Delgado, R. de los Reyes, B. De Lotto, E. Domingo‐Santamaria, D. Dorner, M. Doro, M. Errando, M. Fagiolini, D. Ferenc, E. Fernandez, R. Firpo, J. Flix, M. V. Fonseca, L. Font, M. Fuchs, N. Galante, R. J. Garcia‐Lopez, M. Garczarczyk, M. Gaug, M. Giller, F. Goebel, D. Hakobyan, M. Hayashida, T. Hengstebeck, A. Herrero, D. Hohne, J. Hose, D. Hrupec, C. C. Hsu, P. Jacon, T. Jogler, R. Kosyra, D. Kranich, R. Kritzer, A. Laille, E. Lindfors, S. Lombardi, F. Longo, J. Lopez, M. Lopez, E. Lorenz, P. Majumdar, G. Maneva, K. Mannheim, O. Mansutti, M. Mariotti, M. Martinez, D. Mazin, C. Merck, M. Meucci, M. Meyer, J. M. Miranda, R. Mirzoyan, S. Mizobuchi, A. Moralejo, D. Nieto, K. Nilsson, J. Ninkovic, E. Ona‐Wilhelmi, N. Otte, I. Oya, D. Paneque, M. Panniello, R. Paoletti, J. M. Paredes, M. Pasanen, D. Pascoli, F. Pauss, R. Pegna, M. Persic, L. Peruzzo, A. Piccioli, E. Prandini, N. Puchades, A. Raymers, W. Rhode, M. Ribo, J. Rico, M. Rissi, A. Robert, S. Rugamer, A. Saggion, T. Saito, A. Sanchez, P. Sartori, V. Scalzotto, V. Scapin, R. Schmitt, T. Schweizer, M. Shayduk, K. Shinozaki, S. N. Shore, N. Sidro, A. Sillanpaa, D. Sobczynska, A. Stamerra, L. S. Stark, L. Takalo, F. Tavecchio, P. Temnikov, D. Tescaro, M. Teshima, D. F. Torres, N. Turini, H. Vankov, V. Vitale, R. M. Wagner, T. Wibig, W. Wittek, F. Zandanel, R. Zanin, J. Zapatero
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The Astrophysical Journal
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
The Astrophysical Journal
E-Prints Complutense. Archivo Institucional de la UCM
instname
The blazar Markarian 501 (Mrk 501) was observed at energies above 0.10 TeV with the MAGIC telescope from May through July 2005. The high sensitivity of the instrument enabled the determination of the flux and spectrum of the source on a night-by-nigh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61b192f05e56ce12bba9a65e05311d73
https://doi.org/10.1086/521382
https://doi.org/10.1086/521382
Autor:
J. Albert, E. Aliu, H. Anderhub, P. Antoranz, A. Armada, C. Baixeras, J. A. Barrio, H. Bartko, D. Bastieri, J. Becker, W. Bednarek, K. Berger, C. Bigongiari, A. Biland, R. K. Bock, P. Bordas, V. Bosch‐Ramon, T. Bretz, I. Britvitch, M. Camara, E. Carmona, A. Chilingarian, S. Ciprini, J. A. Coarasa, S. Commichau, J. L. Contreras, J. Cortina, M. T. Costado, V. Curtef, V. Danielyan, F. Dazzi, A. De Angelis, C. Delgado, R. de los Reyes, B. De Lotto, E. Domingo‐Santamaria, D. Dorner, M. Doro, M. Errando, M. Fagiolini, D. Ferenc, E. Fernandez, R. Firpo, J. Flix, M. V. Fonseca, L. Font, M. Fuchs, N. Galante, R. Garcia‐Lopez, M. Garczarczyk, M. Gaug, M. Giller, F. Goebel, D. Hakobyan, M. Hayashida, T. Hengstebeck, A. Herrero, D. Hohne, J. Hose, C. C. Hsu, P. Jacon, T. Jogler, O. Kalekin, R. Kosyra, D. Kranich, R. Kritzer, A. Laille, T. Lenisa, P. Liebing, E. Lindfors, S. Lombardi, F. Longo, J. Lopez, M. Lopez, E. Lorenz, P. Majumdar, G. Maneva, K. Mannheim, O. Mansutti, M. Mariotti, M. Martinez, D. Mazin, C. Merck, M. Meucci, M. Meyer, J. M. Miranda, R. Mirzoyan, S. Mizobuchi, A. Moralejo, K. Nilsson, J. Ninkovic, E. Ona‐Wilhelmi, N. Otte, I. Oya, D. Paneque, M. Panniello, R. Paoletti, J. M. Paredes, M. Pasanen, D. Pascoli, F. Pauss, R. Pegna, M. Persic, L. Peruzzo, A. Piccioli, M. Poller, E. Prandini, N. Puchades, A. Raymers, W. Rhode, M. Ribo, J. Rico, M. Rissi, A. Robert, S. Rugamer, A. Saggion, A. Sanchez, P. Sartori, V. Scalzotto, V. Scapin, R. Schmitt, T. Schweizer, M. Shayduk, K. Shinozaki, S. N. Shore, N. Sidro, A. Sillanpaa, D. Sobczynska, A. Stamerra, L. S. Stark, L. Takalo, P. Temnikov, D. Tescaro, M. Teshima, N. Tonello, D. F. Torres, N. Turini, H. Vankov, V. Vitale, R. M. Wagner, T. Wibig, W. Wittek, R. Zanin, J. Zapatero
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Dipòsit Digital de la UB
Universidad de Barcelona
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
Dipòsit Digital de la UB
Universidad de Barcelona
E-Prints Complutense. Archivo Institucional de la UCM
instname
During its first data cycle, between 2005 and the beginning of 2006, the fast repositioning system of the MAGIC telescope allowed the observation of nine different gamma-ray bursts as possible sources of very high energy gamma-rays. These observation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c379d9d399b409db5f0c889653992b1
https://doi.org/10.1086/520761
https://doi.org/10.1086/520761
Autor:
J.-P. Tavernet, J. Bolmont, Masahiro Teshima, J. Hose, R. Mirzoyan, E. Lorenz, P. Vincent, Hugh Dickinson, M. Kurz, Max Knotig, M. Shayduk
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 695:109-112
The Cherenkov Telescope Array (CTA) is planned as the next generation ground-based instrument (after VERITAS, H.E.S.S. and MAGIC) for astrophysics by means of very high energy γ - rays . The CTA collaboration includes the MAGIC, the H.E.S.S. and the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e76310837cb8912425d162d434ef6a09
https://doi.org/10.1016/j.nima.2011.12.010
https://doi.org/10.1016/j.nima.2011.12.010