no code implementations • 18 Jan 2021 • L. Burderi, T. Di Salvo, A. Sanna, F. Fiore, A. Riggio, A. F. Gambino, the HERMES-TP, HERMES-SP Collaborations
This ratio is as small as 1E-23 for photons in the gamma-ray band (100 keV).
Quantization High Energy Astrophysical Phenomena High Energy Physics - Experiment
no code implementations • 8 Jan 2021 • A. Sanna, A. F. Gambino, L. Burderi, A. Riggio, T. Di Salvo, F. Fiore, M. Lavagna, R. Bertacin, Y. Evangelista, R. Campana, F. Fuschino, P. Lunghi, A. Monge, B. Negri, S. Pirrotta, S. Puccetti, the HERMES-TP, HERMES-SP Collaborations
Moreover, we will quantitatively discuss the all-sky monitor capabilities of the HERMES Pathfinder as well as its achievable accuracies on the localisation of the detected Gamma-Ray Bursts.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics