Zobrazeno 1 - 10
of 473
pro vyhledávání: '"Blondel C"'
Autor:
Simonin, A., Achard, Jocelyn, Achkasov, K., Béchu, S., Baudouin, C., Baulaigue, O., Blondel, C., Boeuf, J. P., Cartry, Gilles, Chaibi, W., Drag, C., de Esch, H. P. L., Fiorucci, D., Fubiani, G., Furno, I., Futtersack, R., Garibaldi, P., Gicquel, A., Grand, C., Guittienne, Ph, Hagelaar, G., Howling, A., Jacquier, R., Kirkpatrick, M. J., Lemoine, D., Lepetit, B., Minea, T., Odic, E., Revel, A., Soliman, B. A., Teste, P.
Publikováno v:
Nuclear Fusion, IOP Publishing, 2015, 55 (12), pp.123020
Since the signature of the ITER treaty in 2006, a new research programme targeting the emergence of a new generation of Neutral Beam (NB) system for the future fusion reactor (DEMO Tokamak) has been underway between several laboratories in Europe. Th
Externí odkaz:
http://arxiv.org/abs/1911.12210
Autor:
Kiener, J., Tatischeff, V., Deloncle, I., de Séréville, N., Laurent, P., Blondel, C., Chabot, M., Chipaux, R., Coc, A., Dubos, S., Gostojic, A., Goutev, N., Hamadache, C., Hammache, F., Horeau, B., Limousin, O., Ouichaoui, S., Prévot, G., Rodríguez-Gasén, R., Yavahchova, M. S.
Publikováno v:
Nucl. Instr. and Meth. in Physics Research A 798, 152 (2015)
The response of a scintillation detector with a cylindrical 1.5-inch LaBr3:Ce crystal to incident neutrons has been measured in the energy range En = 2-12 MeV. Neutrons were produced by proton irradiation of a Li target at Ep = 5-14.6 MeV with pulsed
Externí odkaz:
http://arxiv.org/abs/1512.00305
Autor:
Antier, S., Ferrando, P., Limousin, O., Caroli, E., da Silva, R. M. Curado, Blondel, C., Chipaux, R., Honkimaki, V., Horeau, B., Laurent, P., Maia, J. M., Meuris, A., Del Sordo, S., Stephen, J. B.
Since the initial exploration of soft gamma-ray sky in the 60's, high-energy celestial sources have been mainly characterized through imaging, spectroscopy and timing analysis. Despite tremendous progress in the field, the radiation mechanisms at wor
Externí odkaz:
http://arxiv.org/abs/1505.00976
The Astrophysics Division of CEA Saclay has a long history in the development of CdTe based pixelated detection planes for X and gamma-ray astronomy, with time-resolved imaging and spectrometric capabilities. The last generation, named Caliste HD, is
Externí odkaz:
http://arxiv.org/abs/1502.01491
Autor:
Lebrun, F., Leray, J. -P., Lavocat, P., Cretolle, J., Arques, M., Blondel, C., Bonnin, C., Bouere, A., Cara, C., Chaleil, T., Daly, F., Desages, F., Dzitko, H., Horeau, B., Laurent, P., Limousin, O., Mathy, F., Mauguen, V., Meignier, F., Molinie, F., Poindron, E., Rouger, M., Sauvageon, A., Tourette, T.
Publikováno v:
Astron.Astrophys.411:L141-L148,2003
For the first time in the history of high energy astronomy, a large CdTe gamma-ray camera is operating in space. ISGRI is the low-energy camera of the IBIS telescope on board the INTEGRAL satellite. This paper details its design and its in-flight beh
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310362
Autor:
Terrier, Regis, Lebrun, F., Bazzano, A., Belanger, G., Bird, A. J., Blondel, C., David, P., Goldoni, P., Goldwurm, A., Gros, A., Laurent, P., Malaguti, G., Sauvageon, A., Segreto, A., Ubertini, P.
Publikováno v:
Astron.Astrophys.411:L167-L172,2003
ISGRI, the IBIS low energy camera (15 keV - 1 MeV) on board INTEGRAL, is the first large CdTe gamma-ray imager in orbit. We present here an overview of the ISGRI in-flight calibrations performed during the first months after launch. We discuss the st
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310096
Akademický článek
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Autor:
Attié, D., Blondel, C., Boilevin-Kayl, L., Desforges, D., Ferrer-Ribas, E., Giomataris, I., Gevin, O., Jeanneau, F., Limousin, O., Meuris, A., Papaevangelou, T., Peyaud, A.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 July 2015 787:312-314
Autor:
Meuris, A., Limousin, O., Gevin, O., Blondel, C., Martignac, J., Vassal, M.-C., Soufflet, F., Fiant, N., Bednarzik, M., Stutz, S., Grimm, O., Commichau, V.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 July 2015 787:72-77
Akademický článek
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