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pro vyhledávání: '"Ferro, L"'
Autor:
Guidorzi, C., Maccary, R., Tsvetkova, A., Kobayashi, S., Amati, L., Bazzanini, L., Bulla, M., Camisasca, A. E., Ferro, L., Frederiks, D., Frontera, F., Lysenko, A., Maistrello, M., Ridnaia, A., Svinkin, D., Ulanov, M.
At the dawn of the gamma-ray burst (GRB) afterglow era, a Cepheid-like correlation was discovered between time variability V and isotropic-equivalent peak luminosity Liso of the prompt emission of about a dozen long GRBs with measured redshift availa
Externí odkaz:
http://arxiv.org/abs/2409.01644
Autor:
Maccary, R., Maistrello, M., Guidorzi, C., Sartori, M., Amati, L., Bazzanini, L., Bulla, M., Camisasca, A. E., Ferro, L., Frontera, F., Tsvetkova, A.
Context. The dissipation process responsible for the long gamma-ray burst (GRB) prompt emission and the kind of dynamics that drives the release of energy as a function of time are still key open issues. We recently found that the distribution of the
Externí odkaz:
http://arxiv.org/abs/2407.06002
Autor:
Guidorzi, C., Sartori, M., Maccary, R., Tsvetkova, A., Amati, L., Bazzanini, L., Bulla, M., Camisasca, A. E., Ferro, L., Frontera, F., Li, C. K., Xiong, S. L., Zhang, S. N.
Publikováno v:
A&A 685, A34 (2024)
The variety of long duration gamma-ray burst (LGRB) light curves (LCs) encode a wealth of information on how LGRB engines release energy following the collapse of the progenitor star. Attempts to characterise GRB LCs focused on a number of properties
Externí odkaz:
http://arxiv.org/abs/2402.17282
Autor:
Maccary, R., Guidorzi, C., Amati, L., Bazzanini, L., Bulla, M., Camisasca, A. E., Ferro, L., Frontera, F., Tsvetkova, A.
Discovered more than 50 years ago, gamma-ray burst (GRB) prompt emission remains the most puzzling aspect of GRB physics. Its complex and irregular nature should reveal how newborn GRB engines release their energy. In this respect, the possibility th
Externí odkaz:
http://arxiv.org/abs/2401.14063
Autor:
Campana, R., Evola, C., Labanti, C., Ferro, L., Moita, M., Virgilli, E., Marchesini, E. J., Frontera, F., Rosati, P.
Publikováno v:
Nuclear Inst. and Methods in Physics Research, A 1056 (2023) 168587
A characteristic of every inorganic scintillator crystal is its light yield, i.e., the amount of emitted scintillation photons per unit of energy deposited in the crystal. Light yield is known to be usually non-linear with energy, which impacts the s
Externí odkaz:
http://arxiv.org/abs/2308.06759
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
Akademický článek
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Autor:
Moita, M., Ferro, L., Caroli, E., Cavazzini, L., da Silva, R.M. Curado, Stephen, J.B., Virgilli, E.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A March 2023 1048
