Zobrazeno 1 - 10
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pro vyhledávání: '"Tavani, M"'
The extraordinary gamma-ray burst GRB 221009A provides a great opportunity to investigate the enigmatic origin and evolution of GRBs. However, the complexity of the observations associated with this GRB provides significant challenges to develop a th
Externí odkaz:
http://arxiv.org/abs/2409.02859
Autor:
Pelliciari, D., Bernardi, G., Pilia, M., Naldi, G., Maccaferri, G., Verrecchia, F., Casentini, C., Perri, M., Kirsten, F., Bianchi, G., Bortolotti, C., Bruno, L., Dallacasa, D., Esposito, P., Geminardi, A., Giarratana, S., Giroletti, M., Lulli, R., Maccaferri, A., Magro, A., Mattana, A., Perini, F., Pupillo, G., Roma, M., Schiaffino, M., Setti, G., Tavani, M., Trudu, M., Zanichelli, A.
Fast radio bursts (FRBs) are energetic, millisecond-duration radio pulses observed at extragalactic distances and whose origins are still a subject of heated debate. A fraction of the FRB population have shown repeating bursts, however it's still unc
Externí odkaz:
http://arxiv.org/abs/2405.04802
Autor:
Rizzo, A., Parmiggiani, N., Bulgarelli, A., Macaluso, A., Fioretti, V., Castaldini, L., Di Piano, A., Panebianco, G., Pittori, C., Tavani, M., Sartori, C., Burigana, C., Cardone, V., Farsian, F., Meneghetti, M., Murante, G., Scaramella, R., Schillirò, F., Testa, V., Trombetti, T.
Quantum computing represents a cutting-edge frontier in artificial intelligence. It makes use of hybrid quantum-classical computation which tries to leverage quantum mechanic principles that allow us to use a different approach to deep learning class
Externí odkaz:
http://arxiv.org/abs/2404.14133
Autor:
Parmiggiani, N., Bulgarelli, A., Macaluso, A., Ursi, A., Castaldini, L., Di Piano, A., Falco, R., Fioretti, V., Panebianco, G., Pittori, C., Tavani, M.
AGILE is an Italian Space Agency (ASI) space mission launched in 2007 to study X-ray and gamma-ray phenomena in the energy range from $\sim$20 keV to $\sim$10 GeV. The AGILE AntiCoincidence System (ACS) detects hard-X photons in the 50 - 200 keV ener
Externí odkaz:
http://arxiv.org/abs/2404.02107
Multi-wavelength observations of the lensed quasar PKS 1830$-$211 during the 2019 $\gamma$-ray flare
Autor:
Vercellone, S., Donnarumma, I., Pittori, C., Capitanio, F., De Rosa, A., Di Gesu, L., Kiehlmann, S., Iacolina, M. N., Pellizzoni, P. A., Egron, E., Pacciani, L., Piano, G., Puccetti, S., Righini, S., Valente, G., Verrecchia, F., Vittorini, V., Tavani, M., Brocato, E., Chen, A. W., Hovatta, T., Melis, A., Max-Moerbeck, W., Perrodin, D., Pilia, M., Pili, M., Readhead, A. C. S., Reeves, R., Ridolfi, A., Vitali, F., Bulgarelli, A., Cattaneo, P. W., Lucarelli, F., Morselli, A., Trois, A.
PKS 1830$-$211 is a $\gamma$-ray emitting, high-redshift (z $= 2.507 \pm 0.002$), lensed flat-spectrum radio quasar. During the period mid-February to mid-April 2019, this source underwent a series of strong $\gamma$-ray flares that were detected by
Externí odkaz:
http://arxiv.org/abs/2311.07332
Autor:
Tavani, M., Piano, G., Bulgarelli, A., Foffano, L., Ursi, A., Verrecchia, F., Pittori, C., Casentini, C., Giuliani, A., Longo, F., Panebianco, G., Di Piano, A., Baroncelli, L., Fioretti, V., Parmiggiani, N., Argan, A., Trois, A., Vercellone, S., Cardillo, M., Antonelli, L. A., Barbiellini, G., Caraveo, P., Cattaneo, P. W., Chen, A. W., Costa, E., Del Monte, E., Di Cocco, G., Donnarumma, I., Evangelista, Y., Feroci, M., Gianotti, F., Labanti, C., Lazzarotto, F., Lipari, P., Lucarelli, F., Marisaldi, M., Mereghetti, S., Morselli, A., Pacciani, L., Pellizzoni, A., Perotti, F., Picozza, P., Pilia, M., Rapisarda, M., Rappoldi, A., Rubini, A., Soffitta, P., Trifoglio, M., Vittorini, V., D'Amico, F.
Publikováno v:
ApJL 956 L23, 2023
Gamma-ray emission in the MeV-GeV range from explosive cosmic events is of invaluable relevance to understanding physical processes related to the formation of neutron stars and black holes. Here we report on the detection by the AGILE satellite in t
Externí odkaz:
http://arxiv.org/abs/2309.10515
Autor:
Trudu, M., Pilia, M., Nicastro, L., Guidorzi, C., Orlandini, M., Zampieri, L., Marthi, V. R., Ambrosino, F., Possenti, A., Burgay, M., Casentini, C., Mereminskiy, I., Savchenko, V., Palazzi, E., Panessa, F., Ridolfi, A., Verrecchia, F., Anedda, M., Bernardi, G., Bachetti, M., Burenin, R., Burtovoi, A., Casella, P., Fiori, M., Frontera, F., Gajjar, V., Gardini, A., Ge, M., Guijarro-Román, A., Ghedina, A., Hermelo, I., Jia, S., Li, C., Liao, J., Li, X., Lu, F., Lutivinov, A., Naletto, G., Ochener, P., Papitto, A., Perri, M., Pittori, C., Safanov, B., Semena, A., Strakhov, I., Tavani, M., Ursi, A., Xiong, S. L., Zhang, S. N., Zheltoukhov, S.
Publikováno v:
A&A 676, A17 (2023)
Aims. Fast Radio Bursts are bright radio transients whose origin has not yet explained. The search for a multi-wavelength counterpart of those events can put a tight constrain on the emission mechanism and the progenitor source. Methods. We conducted
Externí odkaz:
http://arxiv.org/abs/2305.18628
Autor:
Parmiggiani, N., Bulgarelli, A., Beneventano, D., Fioretti, V., Di Piano, A., Baroncelli, L., Addis, A., Tavani, M., Pittori, C., Oya, I.
Publikováno v:
Astronomy and Computing, Volume 39, 2022, 100570
In the multi-messenger era, coordinating observations between astronomical facilities is mandatory to study transient phenomena (e.g. Gamma-ray bursts) and is achieved by sharing information with the scientific community through networks such as the
Externí odkaz:
http://arxiv.org/abs/2302.13419
The production site of gamma rays in blazars is closely related to their interaction with the photon fields surrounding the active galactic nucleus. In this work we discuss an indirect method that may help to unveil the presence of ambient structures
Externí odkaz:
http://arxiv.org/abs/2302.10762
Autor:
Parmiggiani, N., Bulgarelli, A., Macaluso, A., Fioretti, V., Di Piano, A., Baroncelli, L., Addis, A., Landoni, M., Pittori, C., Verrecchia, F., Lucarelli, F., Giuliani, A., Longo, F., Beneventano, D., Tavani, M.
AGILE is an ASI space mission launched in 2007 to study X-ray and gamma-ray phenomena in the energy range from $\sim20$ keV to $\sim10$ GeV. The AGILE Team developed a real-time analysis pipeline for the fast detection of transient sources, and the f
Externí odkaz:
http://arxiv.org/abs/2302.10557