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17 yr of Magnetar Bursts Observed with the Fermi Gamma-Ray Burst Monitor

  • Authors: Matt Godwin, Özge Keskin, Mustafa Demirer, Yi-Jing Yi, Lin Lin, Oliver J. Roberts, Ersin Göğüş, Yuki Kaneko, Michael Briggs, Matthew G. Baring, Eric Burns, David M. Palmer, Boyan A. Hristov, Bagrat Mailyan, Christian Malacaria, Eva Palafox, Chryssa Kouveliotou, Alexander J. van der Horst, Peter Veres, George Younes

Matt Godwin et al 2026 The Astrophysical Journal Supplement Series 286 .

  • Provider: AAS Journals

Caption: Figure 6.

The low and high kT distributions for the spectra that prefer BB + BB model. Each prolific magnetar is shown separately in (a) SGR J1935+2154 (N = 75), (b) SGR J1550−5418 (N = 200), (c) SGR 1806−20 (N = 25), and (d) 1E 1841−045 (N = 11). For (a) and (b), the Gaussian fits and means are shown with the curves and the dashed lines, respectively. For (c) and (d), the weighted mean is shown instead due to poor Gaussian fits of low counts.

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