no code implementations • 23 Feb 2021 • F. Ambrosino, A. Miraval Zanon, A. Papitto, F. Coti Zelati, S. Campana, P. D'Avanzo, L. Stella, T. Di Salvo, L. Burderi, P. Casella, A. Sanna, D. de Martino, M. Cadelano, A. Ghedina, F. Leone, F. Meddi, P. Cretaro, M. C. Baglio, E. Poretti, R. P. Mignani, D. F. Torres, G. L. Israel, M. Cecconi, D. M. Russell, M. D. Gonzalez Gomez, A. L. Riverol Rodriguez, H. Perez Ventura, M. Hernandez Diaz, J. J. San Juan, D. M. Bramich, F. Lewis
Millisecond spinning, low magnetic field neutron stars are believed to attain their fast rotation in a 0. 1-1 Gyr-long phase during which they accrete matter endowed with angular momentum from a low-mass companion star.
High Energy Astrophysical Phenomena
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
no code implementations • 8 Jan 2021 • F. Fiore, L. Burderi, M. Lavagna, R. Bertacin, Y. Evangelista, R. Campana, F. Fuschino, P. Lunghi, A. Monge, B. Negri, S. Pirrotta, S. Puccetti, A. Sanna, the HERMES-TP, HERMES-SP Collaborations
HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites Technologic and Scientific Pathfinder) is a constellation of six 3U nano-satellites hosting simple but innovative X-ray detectors, characterized by a large energy band and excellent temporal resolution, and thus optimized for the monitoring of Cosmic High Energy transients such as Gamma Ray Bursts and the electromagnetic counterparts of Gravitational Wave Events, and for the determination of their positions.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics