F
Florian Goebel
Researcher at Max Planck Society
Publications - 120
Citations - 8737
Florian Goebel is an academic researcher from Max Planck Society. The author has contributed to research in topics: MAGIC (telescope) & Telescope. The author has an hindex of 47, co-authored 119 publications receiving 8366 citations. Previous affiliations of Florian Goebel include University of Hamburg & Stony Brook University.
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Journal ArticleDOI
The Super-Kamiokande detector
S. Fukuda,Y. Fukuda,T. Hayakawa,E. Ichihara,M. Ishitsuka,Yoshitaka Itow,Takaaki Kajita,J. Kameda,K. Kaneyuki,S. Kasuga,K. Kobayashi,Y. Kobayashi,Yusuke Koshio,M. Miura,S. Moriyama,Masayuki Nakahata,S. Nakayama,Toshio Namba,Y. Obayashi,A. Okada,M. Oketa,Kimihiro Okumura,T. Oyabu,N. Sakurai,Masato Shiozawa,Yoshihiro Suzuki,Y. Takeuchi,T. Toshito,Y. Totsuka,Shoichi Yamada,S. Desai,M. Earl,J. T. Hong,E. Kearns,M. Masuzawa,M. D. Messier,M. D. Messier,J. L. Stone,L. R. Sulak,C. W. Walter,W. Wang,Kate Scholberg,T. Barszczak,David William Casper,D. W. Liu,W. Gajewski,P. G. Halverson,J. Hsu,W. R. Kropp,S. Mine,L. R. Price,Frederick Reines,M. B. Smy,Henry W. Sobel,M. R. Vagins,K. S. Ganezer,W. E. Keig,R. W. Ellsworth,S. Tasaka,J. W. Flanagan,A. Kibayashi,John G. Learned,S. Matsuno,V. J. Stenger,Y. Hayato,T. Ishii,A. K. Ichikawa,Junichi Kanzaki,T. Kobayashi,T. Maruyama,Koji Nakamura,Y. Oyama,A. Sakai,Makoto Sakuda,Osamu Sasaki,S. Echigo,T. Iwashita,M. Kohama,Atsumu Suzuki,Masaya Hasegawa,T. Inagaki,I. Kato,H. Maesaka,Tsuyoshi Nakaya,K. Nishikawa,Shuji Yamamoto,Todd Haines,Todd Haines,B. K. Kim,R. Sanford,R. Svoboda,E. Blaufuss,M. L. Chen,Z. Conner,Z. Conner,J. A. Goodman,E. Guillian,G. W. Sullivan,D. Turcan,Alec Habig,M. Ackerman,Florian Goebel,J. Hill,J. Hill,C. K. Jung,T. Kato,D. Kerr,Magdalena Malek,K. Martens,C. Mauger,C. McGrew,E. Sharkey,B. Viren,B. Viren,C. Yanagisawa,W. Doki,S. Inaba,K. Ito,M. Kirisawa,M. Kitaguchi,C. Mitsuda,K. Miyano,C. Saji,M. Takahata,M. Takahashi,K. Higuchi,Y. Kajiyama,A. Kusano,Y. Nagashima,K. Nitta,M. Takita,Takashi Yamaguchi,Minoru Yoshida,Hyosun Kim,Soo-Bong Kim,J. Yoo,H. Okazawa,M. Etoh,K. Fujita,Y. Gando,Akira Hasegawa,T. Hasegawa,S. Hatakeyama,Kunio Inoue,K. Ishihara,T. Iwamoto,M. Koga,I. Nishiyama,Hiroshi Ogawa,J. Shirai,A. Suzuki,T. Takayama,F. Tsushima,M. Koshiba,Y. Ichikawa,T. Hashimoto,Y. Hatakeyama,M. Koike,T. Horiuchi,M. Nemoto,K. Nishijima,H. Takeda,H. Fujiyasu,T. Futagami,Hirokazu Ishino,Y. Kanaya,Mikio Morii,H. Nishihama,Hiroaki Nishimura,Toshio Suzuki,Y. Watanabe,D. Kielczewska,D. Kielczewska,U. Golebiewska,H. G. Berns,S. B. Boyd,S. B. Boyd,R. A. Doyle,J. S. George,J. S. George,A. L. Stachyra,A. L. Stachyra,L. Wai,L. Wai,R. J. Wilkes,K. K. Young,H. Kobayashi +186 more
TL;DR: Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons as discussed by the authors, which collected 1678 live-days of data, observing neutrinos from the Sun, Earth's atmosphere, and the K2K long-baseline neutrino beam with high efficiency.
Journal ArticleDOI
Variable very high energy γ-ray emission from markarian 501
Justin Albert,E. Aliu,H. Anderhub,P. Antoranz,A. Armada,C. Baixeras,Juan Abel Barrio,H. Bartko,Denis Bastieri,Julia Becker,W. Bednarek,K. Berger,Ciro Bigongiari,Adrian Biland,R. K. Bock,R. K. Bock,Pol Bordas,Valentí Bosch-Ramon,Thomas Bretz,I. Britvitch,M. Camara,E. Carmona,Ashot Chilingarian,J. A. Coarasa,S. Commichau,Jose Luis Contreras,Juan Cortina,M. T. Costado,V. Curtef,V. Danielyan,Francesco Dazzi,A. De Angelis,C. Delgado,R. de los Reyes,B. De Lotto,E. Domingo-Santamaría,Daniela Dorner,Michele Doro,Manel Errando,Michela Fagiolini,Daniel Ferenc,Enrique Fernández,R. Firpo,Jose Flix,M. V. Fonseca,Ll. Font,M. Fuchs,Nicola Galante,R. J. García-López,M. Garczarczyk,Markus Gaug,Maria Giller,Florian Goebel,D. Hakobyan,Masaaki Hayashida,T. Hengstebeck,A. Herrero,D. Höhne,J. Hose,Dario Hrupec,C. C. Hsu,P. Jacon,T. Jogler,R. Kosyra,D. Kranich,R. Kritzer,A. Laille,Elina Lindfors,Saverio Lombardi,Francesco Longo,J. López,M. López,E. Lorenz,E. Lorenz,P. Majumdar,G. Maneva,K. Mannheim,Oriana Mansutti,Mosè Mariotti,M. I. Martínez,Daniel Mazin,C. Merck,Mario Meucci,M. Meyer,Jose Miguel Miranda,R. Mirzoyan,S. Mizobuchi,Abelardo Moralejo,Daniel Nieto,K. Nilsson,Jelena Ninkovic,E. Oña-Wilhelmi,N. Otte,N. Otte,I. Oya,David Paneque,David Paneque,M. Panniello,Riccardo Paoletti,J. M. Paredes,M. Pasanen,D. Pascoli,F. Pauss,R. Pegna,Massimo Persic,Massimo Persic,L. Peruzzo,A. Piccioli,Elisa Prandini,N. Puchades,A. Raymers,Wolfgang Rhode,Marc Ribó,J. Rico,M. Rissi,A. Robert,S. Rügamer,A. Saggion,Takashi Saito,Alvaro Sanchez,P. Sartori,V. Scalzotto,V. Scapin,R. Schmitt,T. Schweizer,M. Shayduk,M. Shayduk,K. Shinozaki,S. N. Shore,N. Sidro,A. Sillanpää,Dorota Sobczyńska,Antonio Stamerra,L. S. Stark,L. O. Takalo,Fabrizio Tavecchio,Petar Temnikov,D. Tescaro,Masahiro Teshima,Diego F. Torres,Diego F. Torres,Nicola Turini,H. Vankov,V. Vitale,Robert Wagner,Tadeusz Wibig,W. Wittek,F. Zandanel,Roberta Zanin,J. Zapatero +149 more
TL;DR: The MAGIC telescope was used to observe the blazar Markarian 501 (Mrk 501) at energies above 100 GeV from May through July 2005 as mentioned in this paper, and the high sensitivity of the instrument enabled the determination of the flux and spectrum of the source on a night-by-night basis.
Journal ArticleDOI
Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?
J. Albert,E. Aliu,H. Anderhub,L. A. Antonelli,P. Antoranz,Michael Backes,C. Baixeras,Juan Abel Barrio,H. Bartko,Denis Bastieri,J. K. Becker,W. Bednarek,K. Berger,Elisa Bernardini,Ciro Bigongiari,Adrian Biland,R. K. Bock,G. Bonnoli,P. Bordas,Valentí Bosch-Ramon,Thomas Bretz,I. Britvitch,M. Camara,E. Carmona,Ashot Chilingarian,S. Commichau,Jose Luis Contreras,Juan Cortina,M. T. Costado,Stefano Covino,V. Curtef,Francesco Dazzi,A. De Angelis,E. De Cea del Pozo,R. de los Reyes,B. De Lotto,M. De Maria,F. De Sabata,C. Delgado Mendez,Aaron Dominguez,Daniela Dorner,Michele Doro,Manel Errando,Michela Fagiolini,Daniel Ferenc,E. Fernandez,R. Firpo,M. V. Fonseca,Ll. Font,Nicola Galante,R. J. García López,M. Garczarczyk,Markus Gaug,Florian Goebel,M. Hayashida,A. Herrero,D. Höhne,J. Hose,C. C. Hsu,S. Huber,T. Jogler,T. Kneiske,D. Kranich,A. La Barbera,A. Laille,E. Leonardo,Elina Lindfors,Saverio Lombardi,Francesco Longo,M. López,E. Lorenz,P. Majumdar,G. Maneva,N. Mankuzhiyil,K. Mannheim,L. Maraschi,Mosè Mariotti,M. I. Martínez,Daniel Mazin,Mario Meucci,M. S. Meyer,Jose Miguel Miranda,R. Mirzoyan,S. Mizobuchi,Mariano Moles,Abelardo Moralejo,Daniel Nieto,K. Nilsson,Jelena Ninkovic,N. Otte,I. Oya,M. Panniello,Riccardo Paoletti,J. M. Paredes,M. Pasanen,D. Pascoli,F. Pauss,R. Pegna,Miguel A. Pérez-Torres,Massimo Persic,L. Peruzzo,A. Piccioli,Francisco Prada,Elisa Prandini,N. Puchades,A. Raymers,Wolfgang Rhode,Marc Ribó,J. Rico,M. Rissi,A. Robert,S. Rügamer,A. Saggion,Takashi Saito,M. Salvati,Miguel A. Sánchez-Conde,P. Sartori,Konstancja Satalecka,V. Scalzotto,V. Scapin,R. Schmitt,T. Schweizer,M. Shayduk,K. Shinozaki,Steven N. Shore,N. Sidro,Agnieszka Sierpowska-Bartosik,A. Sillanpää,Dorota Sobczyńska,Felix Spanier,Antonio Stamerra,L. S. Stark,L. O. Takalo,Fabrizio Tavecchio,Petar Temnikov,D. Tescaro,Masahiro Teshima,M. Tluczykont,Diego F. Torres,Nicola Turini,H. Vankov,Alessio Venturini,V. Vitale,Robert Wagner,W. Wittek,Victor Zabalza,Fabio Zandanel,Roberta Zanin,J. Zapatero +148 more
TL;DR: The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detected very-high-energy gamma rays from a giant flare of the distant Quasi-Stellar Radio Source 3C 279, at a distance of more than 5 billion light-years.
Journal ArticleDOI
Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303.
Justin Albert,E. Aliu,H. Anderhub,P. Antoranz,A. Armada,M. Asensio,C. Baixeras,Juan Abel Barrio,M. Bartelt,H. Bartko,Denis Bastieri,S. R. Bavikadi,W. Bednarek,K. Berger,Ciro Bigongiari,Adrian Biland,E. Bisesi,R. K. Bock,Pol Bordas,Valentí Bosch-Ramon,Thomas Bretz,I. Britvitch,M. Camara,E. Carmona,Ashot Chilingarian,Stefano Ciprini,J. A. Coarasa,S. Commichau,Jose Luis Contreras,Juan Cortina,V. Curtef,V. Danielyan,Francesco Dazzi,A. De Angelis,R. de los Reyes,B. De Lotto,E. Domingo-Santamaría,Daniela Dorner,Michele Doro,Manel Errando,Michela Fagiolini,Daniel Ferenc,E. Fernandez,R. Firpo,Jose Flix,M. V. Fonseca,Ll. Font,M. Fuchs,Nicola Galante,M. Garczarczyk,Markus Gaug,Maria Giller,Florian Goebel,D. Hakobyan,Masaaki Hayashida,T. Hengstebeck,D. Höhne,J. Hose,C. C. Hsu,Paula Gina Isar,P. Jacon,O. Kalekin,R. Kosyra,D. Kranich,D. Kranich,M. Laatiaoui,A. Laille,T. Lenisa,P. Liebing,Elina Lindfors,S. Lombardi,Francesco Longo,Josue J. Lopez,M. López,E. Lorenz,F. Lucarelli,P. Majumdar,G. Maneva,K. Mannheim,Oriana Mansutti,Mosè Mariotti,M. I. Martínez,K. Mase,Daniel Mazin,C. Merck,Mario Meucci,M. Meyer,Jose Miguel Miranda,R. Mirzoyan,S. Mizobuchi,Abelardo Moralejo,K. Nilsson,E. Oña-Wilhelmi,R. Orduña,N. Otte,I. Oya,David Paneque,Riccardo Paoletti,Josep M. Paredes,M. Pasanen,D. Pascoli,F. Pauss,N. Pavel,R. Pegna,Massimo Persic,L. Peruzzo,A. Piccioli,M. Poller,Guy G. Pooley,Elisa Prandini,A. Raymers,Wolfgang Rhode,Marc Ribó,J. Rico,B. Riegel,M. Rissi,A. Robert,Gustavo E. Romero,S. Rügamer,A. Saggion,Alvaro Sanchez,P. Sartori,V. Scalzotto,V. Scapin,R. Schmitt,T. Schweizer,M. Shayduk,K. Shinozaki,Steven N. Shore,N. Sidro,A. Sillanpää,Dorota Sobczyńska,Antonio Stamerra,L. S. Stark,L. O. Takalo,Petar Temnikov,D. Tescaro,Masahiro Teshima,N. Tonello,A. Torres,Diego F. Torres,Nicola Turini,H. Vankov,V. Vitale,Robert Wagner,Tadeusz Wibig,W. Wittek,R. Zanin,J. Zapatero +148 more
TL;DR: The detection of variable gamma-ray emission above 100 gigaelectron volts from the microquasar LS I 61 + 303 is reported, which suggests that the emission is periodic.
Journal ArticleDOI
Measurement of a small atmospheric νμ/νe ratio
Y. Fukuda,T. Hayakawa,E. Ichihara,Kunio Inoue,K. Ishihara,H. Ishino,Yoshitaka Itow,Takaaki Kajita,J. Kameda,S. Kasuga,Ken-ichiro Kobayashi,Yohei Kobayashi,Yusuke Koshio,K. Martens,M. Miura,Masayuki Nakahata,S. Nakayama,A. Okada,M. Oketa,Ko Okumura,M. Ota,N. Sakurai,Masato Shiozawa,Yasunari Suzuki,Y. Takeuchi,Y. Totsuka,Shinya Yamada,M. Earl,Alec Habig,J. T. Hong,E. Kearns,S. B. Kim,S. B. Kim,M. Masuzawa,M. Masuzawa,M. D. Messier,Kate Scholberg,J. L. Stone,L. R. Sulak,C. W. Walter,M. Goldhaber,T. Barszczak,W. Gajewski,P. G. Halverson,J. Hsu,W. R. Kropp,L. R. Price,Frederick Reines,H. W. Sobel,Mark R. Vagins,K. S. Ganezer,W. E. Keig,R. W. Ellsworth,S. Tasaka,J. W. Flanagan,A. Kibayashi,John G. Learned,S. Matsuno,V. J. Stenger,D. Takemori,T. Ishii,Junichi Kanzaki,T. Kobayashi,K. Nakamura,K. Nishikawa,Yuichi Oyama,A. Sakai,Makoto Sakuda,Osamu Sasaki,S. Echigo,M. Kohama,A. T. Suzuki,Todd Haines,Todd Haines,E. Blaufuss,R. Sanford,R. Svoboda,M. L. Chen,Z. Conner,Z. Conner,J. A. Goodman,G. W. Sullivan,Masaki Mori,Masaki Mori,Florian Goebel,J. Hill,C. K. Jung,C. Mauger,C. McGrew,E. Sharkey,B. Viren,C. Yanagisawa,W. Doki,T. Ishizuka,T. Ishizuka,Y. Kitaguchi,H. Koga,Kazumasa Miyano,H. Okazawa,C. Saji,M. Takahata,A. Kusano,Y. Nagashima,M. Takita,Takashi Yamaguchi,Minoru Yoshida,M. Etoh,K. Fujita,Akira Hasegawa,Takehisa Hasegawa,S. Hatakeyama,T. Iwamoto,T. Kinebuchi,M. Koga,Tomoyuki Maruyama,Hiroshi Ogawa,Masao Saito,A. Suzuki,F. Tsushima,Masatoshi Koshiba,M. Nemoto,Kyoshi Nishijima,T. Futagami,Y. Hayato,Y. Kanaya,K. Kaneyuki,Y. Watanabe,D. Kielczewska,D. Kielczewska,R. A. Doyle,J. S. George,A. L. Stachyra,L. Wai,J. Wilkes,K. K. Young +134 more
TL;DR: In this article, the super-Kamiokande detector was used to detect atmospheric neutrino interactions with momentum p e > 100 MeV/c, p μ > 200 MeV /c, and with visible energy less than 1.33 GeV.