Zobrazeno 1 - 10
of 891
pro vyhledávání: '"T. Kamae"'
Autor:
M. Chauvin, H.-G. Florén, M. Friis, M. Jackson, T. Kamae, J. Kataoka, T. Kawano, M. Kiss, V. Mikhalev, T. Mizuno, N. Ohashi, T. Stana, H. Tajima, H. Takahashi, N. Uchida, M. Pearce
Publikováno v:
Scientific Reports, Vol 7, Iss 1, Pp 1-6 (2017)
Abstract Strong magnetic fields, synchrotron emission, and Compton scattering are omnipresent in compact celestial X-ray sources. Emissions in the X-ray energy band are consequently expected to be linearly polarized. X-ray polarimetry provides a uniq
Externí odkaz:
https://doaj.org/article/bcac59adb6f8425f8f21f6e4f922faaa
Akademický článek
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Autor:
S. GJESDAL, G. PRESSER, T. KAMAE, P. STEFFEN, J. STEINBERGER, F. VANNUCCI, H. WAHL, F. EISELE, H. FILTHUTH, V. LÜTH, G. ZECH, K. KLEINKNECHT
Publikováno v:
Memorial Volume for Jack Steinberger ISBN: 9789811264429
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f4a9e56374fdd580ef8067e8f8e9c355
https://doi.org/10.1142/9789811264436_0015
https://doi.org/10.1142/9789811264436_0015
Akademický článek
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Autor:
Soebur Razzaque, R. Buehler, T. A. Porter, J. Li, Peter F. Michelson, Marcello Giroletti, L. Tibaldo, F. Piron, Denis Bastieri, N. Saggini, N. Di Lalla, G. Tosti, Dario Gasparrini, Francesco Longo, A. Fiori, Stefan Larsson, J. G. Thayer, Ioannis Liodakis, F. Fana Dirirsa, W. B. Atwood, Luca Baldini, J. S. Perkins, M. Ceccanti, Alessandro Brez, D. Serini, Sylvain Guiriec, Stefano Ciprini, Mn Mazziotta, S. Rainò, Tsunefumi Mizuno, G. Foglia, M. Razzano, Johann Cohen-Tanugi, J. Bregeon, Sina Chen, L. Di Venere, Michele Pinchera, T. J. Johnson, Seth Digel, Elliott D. Bloom, F. Loparco, M. N. Lovellette, M.-H. Grondin, F. Gargano, Hiroyasu Tajima, R. Primavera, Ronaldo Bellazzini, J. E. Grove, Yasushi Fukazawa, E. Orlando, M. Lemoine-Goumard, Marco Ajello, E. Rapposelli, Roopesh Ojha, Denise A. Smith, E. Hays, P. M. Saz Parkinson, E. J. Siskind, G. Principe, Manuel Meyer, P. Fusco, N. Menon, Diego F. Torres, Melissa Pesce-Rollins, J. Valverde, Matthew Kerr, Elisabetta Bissaldi, H. Poon, M. Orienti, S. Buson, Vaidehi S. Paliya, D. J. Thompson, D. Fabiani, Carmelo Sgrò, Riccardo Rando, Magnus Axelsson, A. Reimer, Massimo Minuti, S. Maldera, J. J. Russell, Warit Mitthumsiri, R. Bagagli, S. Griffin, F. D'Ammando, T. Kamae, G. Martí-Devesa, Z. Pei, E. Cavazzuti, E. Nuss, David Paneque, P. Spinelli, T. Glanzman, M. Bagni, F. de Palma, Alessandro Paccagnella, M. Kuss, Aaron Dominguez, M. Mongelli, Luca Latronico, Igor V. Moskalenko, Gloria Spandre, N. Scolieri, R. A. Cameron, G. Jóhannesson, Gabrijela Zaharijas, Alberto Manfreda, L. Vigiani, Bindu Rani, P. Bruel, Ismaël Cognard, Olaf Reimer, D. Horan, P. de la Torre Luque, L. Guillemot, M. E. Monzani, F. Bellardi, Elizabeth C. Ferrara, David A. Green, I. Mereu, P. Caraveo, S. Cutini, D. J. Suson, C. C. Cheung, R. Bonino, P. Lubrano, M. Gustafsson, J. L. Racusin, M. Negro
Publikováno v:
Astrophysical Journal Supplement
Astrophysical Journal Supplement, American Astronomical Society, 2021, 256 (1), pp.12. ⟨10.3847/1538-4365/ac0ceb⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astrophysical Journal Supplement, American Astronomical Society, 2021, 256 (1), pp.12. ⟨10.3847/1538-4365/ac0ceb⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
The Large Area Telescope (LAT), the primary instrument for the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from 30 MeV to more than 300 GeV. We describ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::caf9c4f29603e10478fccf51427cf893
http://arxiv.org/abs/2106.12203
http://arxiv.org/abs/2106.12203
Autor:
S. Abdollahi, F. Acero, M. Ackermann, M. Ajello, W. B. Atwood, M. Axelsson, L. Baldini, J. Ballet, G. Barbiellini, D. Bastieri, J. Becerra Gonzalez, R. Bellazzini, A. Berretta, E. Bissaldi, R. D. Blandford, E. D. Bloom, R. Bonino, E. Bottacini, T. J. Brandt, J. Bregeon, P. Bruel, R. Buehler, T. H. Burnett, S. Buson, R. A. Cameron, R. Caputo, P. A. Caraveo, J. M. Casandjian, D. Castro, E. Cavazzuti, E. Charles, S. Chaty, S. Chen, C. C. Cheung, G. Chiaro, S. Ciprini, J. Cohen-Tanugi, L. R. Cominsky, J. Coronado-Blázquez, D. Costantin, A. Cuoco, S. Cutini, F. D’Ammando, M. DeKlotz, P. de la Torre Luque, F. de Palma, A. Desai, S. W. Digel, N. Di Lalla, M. Di Mauro, L. Di Venere, A. Domínguez, D. Dumora, F. Fana Dirirsa, S. J. Fegan, E. C. Ferrara, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, D. Green, I. A. Grenier, S. Griffin, M.-H. Grondin, J. E. Grove, S. Guiriec, A. K. Harding, K. Hayashi, E. Hays, J. W. Hewitt, D. Horan, G. Jóhannesson, T. J. Johnson, T. Kamae, M. Kerr, D. Kocevski, M. Kovac’evic’, M. Kuss, D. Landriu, S. Larsson, L. Latronico, M. Lemoine-Goumard, J. Li, I. Liodakis, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, S. Maldera, D. Malyshev, A. Manfreda, E. J. Marchesini, L. Marcotulli, G. Martí-Devesa, P. Martin, F. Massaro, M. N. Mazziotta, J. E. McEnery, I. Mereu, M. Meyer, P. F. Michelson, N. Mirabal, T. Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, M. Negro, E. Nuss, R. Ojha, N. Omodei, M. Orienti, E. Orlando, J. F. Ormes, M. Palatiello, V. S. Paliya, D. Paneque, Z. Pei, H. Peña-Herazo, J. S. Perkins, M. Persic, M. Pesce-Rollins, V. Petrosian, L. Petrov, F. Piron, H. Poon, T. A. Porter, G. Principe, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, Q. Remy, T. Reposeur, R. W. Romani, P. M. Saz Parkinson, F. K. Schinzel, D. Serini, C. Sgrò, E. J. Siskind, D. A. Smith, G. Spandre, P. Spinelli, A. W. Strong, D. J. Suson, H. Tajima, M. N. Takahashi, D. Tak, J. B. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, E. Torresi, J. Valverde, B. Van Klaveren, P. van Zyl, K. Wood, M. Yassine, G. Zaharijas
Publikováno v:
Astrophys.J.Suppl.
Astrophys.J.Suppl., 2020, 247 (1), pp.33. ⟨10.3847/1538-4365/ab6bcb⟩
The astrophysical journal / Supplement series 247(1), 33 (2020). doi:10.3847/1538-4365/ab6bcb
Digital.CSIC. Repositorio Institucional del CSIC
instname
The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, IOPscience 2020, 247 (1), pp.33. ⟨10.3847/1538-4365/ab6bcb⟩
Astrophys.J.Suppl., 2020, 247 (1), pp.33. ⟨10.3847/1538-4365/ab6bcb⟩
The astrophysical journal / Supplement series 247(1), 33 (2020). doi:10.3847/1538-4365/ab6bcb
Digital.CSIC. Repositorio Institucional del CSIC
instname
The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, IOPscience 2020, 247 (1), pp.33. ⟨10.3847/1538-4365/ab6bcb⟩
We present the fourth Fermi Large Area Telescope catalog (4FGL) of γ-ray sources. Based on the first eight years of science data from the Fermi Gamma-ray Space Telescope mission in the energy range from 50 MeV to 1 TeV, it is the deepest yet in this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55cb772d5c4d5cdada12ac313b50b093
https://hal.archives-ouvertes.fr/hal-02309079
https://hal.archives-ouvertes.fr/hal-02309079
Publikováno v:
CAMX 2019.
Akademický článek
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Autor:
Mark Pearce, Mette Friis, Maxime Chauvin, H. G. Floren, Nagomi Uchida, Hiromitsu Takahashi, Mózsi Kiss, M. Jackson, N. Ohashi, Theodor-Adrian Stana, T. Kawano, Tsunefumi Mizuno, H. Tajima, Victor Mikhalev, T. Kamae, Jun Kataoka
Publikováno v:
Scientific Reports, Vol 8, Iss 1, Pp 1-1 (2018)
Scientific Reports
Scientific Reports
Strong magnetic fields, synchrotron emission, and Compton scattering are omnipresent in compact celestial X-ray sources. Emissions in the X-ray energy band are consequently expected to be linearly polarized. X-ray polarimetry provides a unique diagno
Autor:
Tsunefumi Mizuno, H. Tajima, Hiromitsu Takahashi, Miranda Jackson, T. Kawano, Mette Friis, Victor Mikhalev, Mark Pearce, Maxime Chauvin, Mózsi Kiss, T. Kamae, H. G. Floren, Nagomi Uchida, Jun Kataoka
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters.
The linear polarisation fraction and angle of the hard X-ray emission from the Crab provide unique insight into high energy radiation mechanisms, complementing the usual imaging, timing and spectroscopic approaches. Results have recently been present