Zobrazeno 1 - 10
of 128
pro vyhledávání: '"J.-P Dezalay"'
Autor:
Olivier Godet, J.-L Atteia, C. Amoros, P. Roger, L. Bouchet, J.-P Dezalay, M. Yassine, B. Arcier, S. Bordon, K. Lacombe, E. Lecomte, M. Llamas, S. Maestre, W. Marty, Stéphane Papais, P. Ramon, C. Verdeil, V. Waegebaert, S. Schanne, N. Dagoneau, F. Chateau, P. Kestener, H. Le Provost, C. Tahoulan, B. Cordier, Th. Tourrette, F. Daly, H. Triou, A. Coleiro, A. Goldwurm, C. Lachaud, P. Guillemot, J-M. Mouret, M.-C. Charmeau, L. Perraud, F. Bousquet, Y. Cervantes, Ph. Gasc, H. Pasquier, L. Perrin, M. Ruellan, O. Simonella, M. Yadallee
Publikováno v:
Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray.
Autor:
Armelle Bajat, K. Lacombe, Sujay Mate, Jean-Luc Atteia, B. Houret, V. Waegebaert, Philippe Guillemot, Henri Triou, F. Lebrun, C. Amoros, J.-P. Dezalay, Laurent Bouchet, R. Pons
Publikováno v:
Exper.Astron.
Exper.Astron., 2019, 47 (1-2), pp.245-269. ⟨10.1007/s10686-019-09626-y⟩
Exper.Astron., 2019, 47 (1-2), pp.245-269. ⟨10.1007/s10686-019-09626-y⟩
We discuss the need for very large detection planes for the detection of hard X-ray transients in the multi-messenger era that started with the quasi-simultaneous detection of GRB~170817A by \textit{Fermi}/GBM and \textit{INTEGRAL}/SPI on one hand an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a5c9fce18e436d0ede72033d80f1069
https://hal.archives-ouvertes.fr/hal-02154140
https://hal.archives-ouvertes.fr/hal-02154140
Autor:
J.-P. Dezalay, C. Amoros, K. Lacombe, B. Houret, I. Belkacem, P. Ramon, V. Waegebaert, R. Pons
Publikováno v:
2018 IEEE SENSORS.
ECLAIRs, a 2-D coded-mask imaging camera on-board the Sino-French SVOM space mission, will detect and locate Gamma-ray bursts (GRBs) in near real time in the 4×150 keV energy band. The design of ECLAIRs is driven by the objective of a 4 keV low-ener
Publikováno v:
Astron.Astrophys.
Astron.Astrophys., 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astron.Astrophys., 2018, 610, pp.A58. 〈10.1051/0004-6361/201731875〉
Astron.Astrophys., 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astron.Astrophys., 2018, 610, pp.A58. 〈10.1051/0004-6361/201731875〉
Context. Gravitational wave interferometers have proven the existence of a new class of binary black hole (BBH) weighing tens of solar masses, and have provided the first reliable measurement of the rate of coalescing black holes (BHs) in the local U
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4677daf06c26345b2dbb287060b3a591
https://hal.archives-ouvertes.fr/hal-01730089
https://hal.archives-ouvertes.fr/hal-01730089
Autor:
B. Houret, O. Gevin, O. Godet, K. Lacombe, C. Amoros, P. Ramon, V. Waegebaert, B. Cordier, Jean-Luc Atteia, Ph. Guillemot, F. Gonzalez, J.-P. Dezalay, Olivier Limousin, L. Bouchet, R. Pons
Publikováno v:
Astropart.Phys.
Astropart.Phys., 2018, 103, pp.131-141. ⟨10.1016/j.astropartphys.2018.08.002⟩
Astropart.Phys., 2018, 103, pp.131-141. ⟨10.1016/j.astropartphys.2018.08.002⟩
The hard X-ray imager of the Sino-French SVOM mission, called ECLAIRs, is dedicated to the detection and near real time localization of cosmic transients in the 4 − 150 keV energy range. ECLAIRs is a wide-field camera using a detection plane consis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eaa33b2db6a58b0459239d9b1088c242
https://hal.archives-ouvertes.fr/hal-01876140
https://hal.archives-ouvertes.fr/hal-01876140
Autor:
D. D. Frederiks, A. Tsvetkova, Frédéric Daigne, J.-P. Dezalay, Y. Zolnierowski, Alain Klotz, Jean-Luc Atteia, Damien Turpin, Robert Mochkovitch, V. Heussaff
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2017, 837 (2), pp.119. ⟨10.3847/1538-4357/aa5ffa⟩
The Astrophysical Journal, American Astronomical Society, 2017, 837 (2), pp.119. ⟨10.3847/1538-4357/aa5ffa⟩
The most energetic gamma-ray bursts (GRBs) are remarkable sources releasing huge amounts of energy on short timescales. Their prompt emission, which usually lasts few seconds, is so bright that it is visible across the whole observable universe. Stud
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd9cbb69f97adf541a185df39ac7d49c
http://arxiv.org/abs/1702.02961
http://arxiv.org/abs/1702.02961
Autor:
K. Lacombe, K. Mercier, P. Ramon, M. Galliano, C. Amoros, Marc Billot, J.-P. Dezalay, B. Cordier, J. L. Atteia, B. Houret, O. Godet, V. Waegebaert, Ph. Guillemot, S. Bordon, Kévin Aubaret, R. Pons, Olivier Limousin, O. Gevin, F. Gonzalez, Damien Rambaud, S. Delaigue, G. Nasser
Publikováno v:
SPIE Proceedings.
ECLAIRs, a 2-D coded-mask imaging camera on-board the Sino-French SVOM space missi on, will detect and locate gamma-ray bursts in near real time in the 4 - 150 keV energy band in a large field of view. The design of ECLAIRs has been driven by the obj
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2016, 831 (1), ⟨10.3847/0004-637X/831/1/28⟩
The Astrophysical Journal, 2016, 831 (1), ⟨10.3847/0004-637X/831/1/28⟩
The Astrophysical Journal, American Astronomical Society, 2016, 831 (1), ⟨10.3847/0004-637X/831/1/28⟩
The Astrophysical Journal, 2016, 831 (1), ⟨10.3847/0004-637X/831/1/28⟩
Measuring gamma-ray burst (GRB) properties in their rest-frame is crucial to understand the physics at work in gamma-ray bursts. This can only be done for GRBs with known redshift. Since redshifts are usually measured from the optical spectrum of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aafd3d8a7f31c8db36ea82cd45301247
http://arxiv.org/abs/1605.01303
http://arxiv.org/abs/1605.01303
Autor:
Masaru Matsuoka, Toru Tamagawa, Rie Sato, T. Q. Donaghy, Alan M. Levine, Donald Q. Lamb, Geoffrey B. Crew, Jean François Olive, M. Boer, Nicolas Vasquez Pazmino, Katsuaki Asano, T. Sakamoto, Yujin E. Nakagawa, Carlo Graziani, A. Pelangeon, J. P. Dezalay, Takashi Shimokawabe, Atsumasa Yoshida, Nat Butler, John P. Doty, Kevin Hurley, George R. Ricker, Makoto Arimoto, R. K. Manchanda, Satoshi Sugita, Motoko Suzuki, Gregory Y. Prigozhin, João Braga, G. Pizzichini, J. Garrett Jernigan, Nobuyuki Kawai, Roland Vanderspek, E. E. Fenimore, Joel Villasenor, Yuji Shirasaki, M. Galassi, Jean-Luc Atteia, S. E. Woosley, Ichiro Takahashi
Publikováno v:
Scopus-Elsevier
Using a pulse-fit method, we investigate the spectral lags between the traditional gamma-ray band (50-400 keV) and the X-ray band (6-25 keV) for 8 GRBs with known redshifts (GRB 010921, GRB 020124, GRB 020127, GRB 021211, GRB 030528, GRB 040924, GRB
Autor:
A. Tsvetkova, Damien Turpin, Frédéric Daigne, Robert Mochkovitch, Jean-Luc Atteia, Alain Klotz, Y. Zolnierowski, D. Frederiks, J.-P. Dezalay, V. Heussaff
Publikováno v:
The Astrophysical Journal. 852:144