no code implementations • 26 Jan 2021 • J. Rodi, A. Tramacere, F. Onori, G. Bruni, C. Sánchez-Fernández, M. Fiocchi, L. Natalucci, P. Ubertini
Spectral analysis of the hard X-rays found a \(kT_e \sim 30 \) keV and \( \tau \sim 2\) with a \texttt{CompTT} model, indicative of an accreting black hole binary in the hard state.
High Energy Astrophysical Phenomena
no code implementations • 13 Jan 2021 • D. Svinkin, D. Frederiks, K. Hurley, R. Aptekar, S. Golenetskii, A. Lysenko, A. V. Ridnaia, A. Tsvetkova, M. Ulanov, T. L. Cline, I. Mitrofanov, D. Golovin, A. Kozyrev, M. Litvak, A. Sanin, A. Goldstein, M. S. Briggs, C. Wilson-Hodge, A. von Kienlin, X. -L. Zhang, A. Rau, V. Savchenko, E. Bozzo, C. Ferrigno, P. Ubertini, A. Bazzano, J. C. Rodi, S. Barthelmy, J. Cummings, H. Krimm, D. M. Palmer, W. Boynton, C. W. Fellows, K. P. Harshman, H. Enos, R. Starr
Apart from the huge initial pulses of magnetar giant flares, no astrophysical signal with this combination of temporal and spectral properties and implied energy has been reported previously.
High Energy Astrophysical Phenomena
