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NICER View of the 2020 Burst Storm and Persistent Emission of SGR 1935+2154

  • Authors: George Younes, Tolga Güver, Chryssa Kouveliotou, Matthew G. Baring, Chin-Ping Hu, Zorawar Wadiasingh, Beste Begiçarslan, Teruaki Enoto, Ersin Göğüş, Lin Lin, Alice K. Harding, Alexander J. van der Horst, Walid A. Majid, Sebastien Guillot, and Christian Malacaria

2020 The Astrophysical Journal Letters 904 L21.

  • Provider: AAS Journals

Caption: Figure 2.

Left panels: three examples of bursts emitted during the burst forest plotted with 16 ms resolution in the 1–10 keV energy range. The vertical dotted lines delimit the T100 start and end times of the bursts. The dotted–dashed lines delimit the start and end times of the T90 interval. The peak time of the bursts is shown as a dashed line and corresponds to t = 0. Right panels: spectra of each of the bursts. Panels (a) show the data in FE space and the best-fit absorbed BB model. Panels (b) are the corresponding residuals in terms of σ. Panels (c) show the residuals of an absorbed PL model for comparison. See text for details.

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