Fig. 7
Gamma-ray/optical flux–flux evolution over flare B. LAT 2-day binned fluxes are interpolated to the times of R-band measurements as explained in Sect. 4.1 and plotted on the y-axis. R-band fluxes are plotted on the x-axis. For clarity their errors (typically 5−10% or less) are not shown. Approximate times in days (from MJD 55 322) are indicated along the track.
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