Zobrazeno 1 - 10
of 144
pro vyhledávání: '"Moita M"'
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
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
Autor:
Moita, M., Caroli, E., Maia, J.M., Curado da Silva, R.M., Auricchio, N., Stephen, J.B., Páscoa, M., Trindade, A.M.F.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 February 2019 918:93-98
Autor:
den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Plasse, C., Götz, D., Meuris, A., Ferrando, P., Burwitz, V., Doumayrou, E., Lortholary, M., Moita, M., Mercier, K., Pinsard, F., Prieur, M., Renaud, D., Robinet, F., Schneider, B., Visticot, F.
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13093 Issue: 1 p130931V-130931V-14, 12962184p
Autor:
Simões, N., Maia, J.M., Curado da Silva, R.M., Ghithan, S., Crespo, P., do Carmo, S.J.C., Alves, Francisco, Moita, M., Auricchio, N., Caroli, E.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 January 2018 877:183-191
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.
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
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
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.
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
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