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 Letters904L21.
Provider: AAS Journals
Caption: Figure 4.
Time to peak (Ttp; left panel), time from peak (Tfp; middle panel), and ratio Ttp/Tfp (right panel) distributions. The best-fit lognormal function to each distribution is shown as a black solid line with a mean of 510, 680, and 0.69, respectively.