2017 The Astrophysical Journal Supplement Series23217.
Provider: AAS Journals
Caption: Figure 5.
Fluence distributions of SGR 1806−20 (left) and SGR 1900+14 (right) bursts. Fits are calculated with the COMPT model with PCA fluence shown in black and HEXTE in red. Dashed lines represent Gaussian fits to the fluence distributions.