Zobrazeno 1 - 10
of 343
pro vyhledávání: '"Dezalay, J P."'
Autor:
Ioppolo, S., Kanuchová, Z., James, R. L., Dawes, A., Ryabov, A., Dezalay, J., Jones, N. C., Hoffmann, S. V., Mason, N. J., Strazzulla, G.
Publikováno v:
A&A 646, A172 (2021)
Carbonic acid (H2CO3) is a weak acid relevant to astrobiology which, to date, remains undetected in space. Experimental work has shown that the beta-polymorph of H2CO3 forms under space relevant conditions through energetic (UV photon, electron, and
Externí odkaz:
http://arxiv.org/abs/2012.14863
Akademický článek
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Autor:
Lacombe, K., Amoros, C., Atteia, J. -L., Bajat, A., Bouchet, L., Dezalay, J. -P., Guillemot, P., Houret, B., Lebrun, F., Mate, S., Pons, R., Triou, H., Waegebaert, V.
Publikováno v:
Exp Astron (2019) 47: 245
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:
http://arxiv.org/abs/1909.09015
Publikováno v:
A&A 610, A58 (2018)
Gravitational wave interferometers have proved the existence of a new class of binary black holes (BBHs) weighting tens of solar masses and they have provided the first reliable measurement of the rate of coalescing black holes (BHs) in the local uni
Externí odkaz:
http://arxiv.org/abs/1711.06122
Autor:
Atteia, J-L., Heussaff, V., Dezalay, J. -P., Klotz, A., Turpin, D., Tsvetkova, A. E., Frederiks, D. D., Zolnierowski, Y., Daigne, F., Mochkovitch, R.
Publikováno v:
ApJ 837, 119 (2017)
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:
http://arxiv.org/abs/1702.02961
Measuring 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 afterglow, correl
Externí odkaz:
http://arxiv.org/abs/1503.02760
Autor:
Arimoto, M., Kawai, N., Asano, K., Hurley, K., Suzuki, M., Nakagawa, Y. E., Shimokawabe, T., Pazmino, N. V., Sato, R., Matsuoka, M., Yoshida, A., Tamagawa, T., Shirasaki, Y., Sugita, S., Takahashi, I., Atteia, J. -L., Pelangeon, A., Vanderspek, R., Graziani, C., Prigozhin, G., Villasenor, J., Jernigan, J. G., Crew, G. B., Sakamoto, T., Ricker, G. R., Woosley, S. E., Butler, N., Levine, A., Doty, J. P., Donaghy, T. Q., Lamb, D. Q., Fenimore, E., Galassi, M., Boer, M., Dezalay, J. -P., Olive, J. -F., Braga, J., Manchanda, R., Pizzichini, G.
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
Externí odkaz:
http://arxiv.org/abs/1002.3849
Autor:
Lacombe, K., Dezalay, J-P., Houret, B., Amoros, C., Atteia, J-L., Bouchet, L., Cordier, B., Gevin, O., Godet, O., Gonzalez, F., Guillemot, Ph., Limousin, O., Pons, R., Ramon, P., Waegebaert, V.
Publikováno v:
In Astroparticle Physics December 2018 103:131-141
Autor:
Pélangeon, A., Atteia, J. -L., Nakagawa, Y. E., Hurley, K., Yoshida, A., Vanderspek, R., Suzuki, M., Kawai, N., Pizzichini, G., Boër, M., Braga, J., Crew, G., Donaghy, T. Q., Dezalay, J. P., Doty, J., Fenimore, E. E., Galassi, M., Graziani, C., Jernigan, J. G., Lamb, D. Q., Levine, A., Manchanda, J., Martel, F., Matsuoka, M., Olive, J. -F., Prigozhin, G., Ricker, G. R., Sakamoto, T., Shirasaki, Y., Sugita, S., Takagishi, K., Tamagawa, T., Villasenor, J., Woosley, S. E., Yamauchi, M.
Publikováno v:
Astron.Astrophys.491:157-171,2008
Aims: Taking advantage of the forthcoming Catalog of the HETE-2 mission, the aim of this paper is to evaluate the main properties of HETE-2 GRBs - the E_peak, the T_90 and the E_iso - in their source frames and to derive their unbiased distribution.
Externí odkaz:
http://arxiv.org/abs/0811.3304
Autor:
Stratta, G., Basa, S., Butler, N., Atteia, J. L., Gendre, B., Pelangeon, A., Malacrino, F., Mellier, Y., Kann, D. A., Klose, S., Zeh, A., Masetti, N., Palazzi, E., Gorosabel, J., Castro-Tirado, A. J., Postigo, A. de Ugarte, Jelinek, M., Cepa, J., Castaneda, H., Martinez-Delgado, D., Boer, M., Braga, J., Crew, G., Donaghy, T. Q., Dezalay, J. -P., Doty, J., Fenimore, E. E., Galassi, M., Graziani, C., Jernigan, J. G., Kawai, N., Lamb, D. Q., Levine, A., Manchanda, J., Martel, F., Matsuoka, M., Nakagawa, Y., Olive, J. -F., Pizzichini, G., Prigozhin, G., Ricker, G., Sakamoto, T., Shirasaki, Y., Sugita, S., Suzuki, M., Takagishi, K., Tamagawa, T., Vanderspek, R., Villasenor, J., Woosley, S. E., Yamauchi, M., Yoshida, A.
Publikováno v:
Astron.Astrophys. 461 (2007) 485-492
In this work, we present a multi-wavelength study of XRF 040912, aimed at measuring its distance scale and the intrinsic burst properties. We performed a detailed spectral and temporal analysis of both the prompt and the afterglow emission and we est
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610157