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Three-stage Collapse of the Long Gamma-Ray Burst from GRB 160625B Prompt Multiwavelength Observations

Authors: V. M. Lipunov, V. A. Sadovnichy, M. I. Panasyuk, I. V. Yashin, S. I. Svertilov, S. G. Simakov, D. Svinkin, E. Gorbovskoy, G. V. Lipunova, V. G. Kornilov, D. Frederiks, V. Topolev, R. Rebolo, M. Serra, N. Tiurina, E. Minkina, V. V. Bogomolov, A. V. Bogomolov, A. F. Iyudin, A. Chasovnikov, A. Gabovich, A. Tsvetkova, N. M. Budnev, O. A. Gress, G. Antipov, I. Gorbunov, D. Vlasenko, P. Balanutsa, R. Podesta, K. Zhirkov, A. Kuznetsov, V. Vladimirov, F. Podesta, C. Francile, Yu. Sergienko, A. Tlatov, O. Ershova, D. Cheryasov, V. Yurkov, A. V. Krylov

V. M. Lipunov et al 2023 The Astrophysical Journal 943 .

Provider: AAS Journals

Caption: Figure 4.

The top panel represents the GBM/Fermi counting rate vs. time in the 20–80, 80–300, and 300–1000 keV energy ranges, and the bottom panel represents the light curve from the BDRG1 (NaI detector) 35–170 keV channel cleaned from electron flux background variations, i.e., the zero counts correspond to the mean background level. The green dashed line represents the GBM/Fermi trigger (22:51:16 UT).

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