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P. Esposito et al.
Fig. 3.6 Spectral evolution of SGR 0418+5729 with time during the outburst started in 2009 June
(the time of the detection of the first burst is MJD 54987.9 ≡ TJD 14987.9). Top panel: flux
evolution for the absorbed 0.5–10 keV flux (black), and for the bolometric unabsorbed flux (red).
Middle and bottom panels: evolution of the blackbody temperature and radius, calculated at infinity
and assuming a distance of 2 kpc (from Rea et al. [185])
P. Esposito et al.
Fig. 3.6 Spectral evolution of SGR 0418+5729 with time during the outburst started in 2009 June
(the time of the detection of the first burst is MJD 54987.9 ≡ TJD 14987.9). Top panel: flux
evolution for the absorbed 0.5–10 keV flux (black), and for the bolometric unabsorbed flux (red).
Middle and bottom panels: evolution of the blackbody temperature and radius, calculated at infinity
and assuming a distance of 2 kpc (from Rea et al. [185])