Zobrazeno 1 - 10
of 442
pro vyhledávání: '"Sordo S"'
Autor:
Auricchio, N., Ferro, L., Stephen, J. B., Caroli, E., Virgilli, E., Limousin, O., Moita, M., Gutierrez, Y., Geoffrey, D., Breton, R. Le, Meuris, A., Del Sordo, S., Frontera, F., Rosati, P., Ferrari, C., Lolli, R., Gargano, C., Squerzanti, S.
In astrophysics, several key questions in the hard X soft Gamma-ray range (above 100 keV) require sensitivity and angular resolution that are hardly achievable with current technologies. Therefore, a new kind of instrument able to focus hard X and ga
Externí odkaz:
http://arxiv.org/abs/2301.10728
Autor:
Virgilli, E., Frontera, F., Rosati, P., Guidorzi, C., Ferro, L., Moita, M., Orlandini, M., Fuschino, F., Campana, R., Labanti, C., Marchesini, E., Caroli, E., Auricchio, N., Stephen, J. B., Ferrari, C., Squerzanti, S., Del Sordo, S., Gargano, C., Pucci, M.
Gamma-ray astronomy is a branch whose potential has not yet been fully exploited. The observations of elemental and isotopic abundances in supernova (SN) explosions are key probes not only of the stellar structure and evolution but also for understan
Externí odkaz:
http://arxiv.org/abs/2211.16916
Autor:
Ferro, L, Moita, M., Rosati, P., Lolli, R., Guidorzi, C., Frontera, F., Virgilli, E., Caroli, E., Auricchio, N., Stephen, J. B., Labanti, C., Fuschino, F., Campana, R., Ferrari, C., Squerzanti, S., Pucci, M., del Sordo, S., Gargano, C.
Hard X-/soft Gamma-ray astronomy is a key field for the study of important astrophysical phenomena such as the electromagnetic counterparts of gravitational waves, gamma-ray bursts, black holes physics and many more. However, the spatial localization
Externí odkaz:
http://arxiv.org/abs/2211.16880
Autor:
Auricchio, N., Abbene, L., Benassi, G., Bettelli, M., Buttacavoli, A., Del Sordo, S., Principato, F., Sarzi Amadè, N., Stephen, J.B., Zambelli, N., Zanettini, S., Zappettini, A., Caroli, E.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A February 2023 1047
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
Publikováno v:
In International Journal of Disaster Risk Reduction January 2020 42
Autor:
Malaguti, G., Pareschi, G., Ferrando, P., Caroli, E., Di Cocco, G., Foschini, L., Basso, S., Del Sordo, S., Fiore, F., Bonati, A., Lesci, G., Poulsen, J. M., Monzani, F., Stevoli, A., Negri, B.
The 10-100 keV region of the electromagnetic spectrum contains the potential for a dramatic improvement in our understanding of a number of key problems in high energy astrophysics. A deep inspection of the universe in this band is on the other hand
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509010
Autor:
Masetti, N., Orlandini, M., Fiume, D. Dal, Del Sordo, S., Amati, L., Frontera, F., Palazzi, E., Santangelo, A.
A pointed observation on the galactic high-mass X-ray binary 4U 0114+65 was carried out with BeppoSAX in order to compare the X-ray spectral and timing characteristics observed by this satellite over the broadest range of energies ever (1.5-100 keV)
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508451
Autor:
Amati, L., Frontera, F., Zand, J. J. M. in 't, Capalbi, M., Landi, R., Soffitta, P., Vetere, L., Antonelli, L. A., Costa, E., Del Sordo, S., Feroci, M., Guidorzi, C., Heise, J., Masetti, N., Montanari, E., Nicastro, L., Palazzi, E., Piro, L.
Publikováno v:
Astron.Astrophys. 426 (2004) 415-423
We report on the X-ray observations of the X-ray flash (XRF) which occurred on 2002 April 27, three days before BeppoSAX was switched off. The event was detected with the BeppoSAX Wide Field Cameras but not with the Gamma ray Burst Monitor. A follow-
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407166
Autor:
Masetti, N., Foschini, L., Palazzi, E., Beckmann, V., Lund, N., Brandt, S., Westergaard, N. J., Amati, L., Caroli, E., Del Sordo, S., Di Cocco, G., Durouchoux, P., Farinelli, R., Frontera, F., Orlandini, M., Zdziarski, A.
Publikováno v:
Astron.Astrophys. 423 (2004) 651-656
Here we report results of an INTEGRAL-AO1 observation of the X-ray burst and atoll source Ser X-1 performed in May 2003. The object was observed for a total on-source time of 400 ks but nearly 8 degrees off-axis due to its amalgamation with an observ
Externí odkaz:
http://arxiv.org/abs/astro-ph/0405277