Fig. 11
SED of Flare B. L′-, Ks-band, and X-ray peak fluxes are plotted in red, orange, and blue, respectively. NIR error bars account for the uncertainty in the extinction correction. The 1–100 GeV spectrum of 1FGL J1745.6–2900 is indicated in dark gray. Models SSC1, SSC2, and SB correspond to the green dashed, magenta solid, black dash-dot lines, respectively.
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