Fig. 14
Simultaneous X-ray, NIR and radio observations of flare I/1 from Sgr A* on 2014 Mar. 10. Top panel: the EPIC/pn smoothed light curve computed with a window width of 500 s and its error in gray. The dashed lines are the Bayesian blocks. Middle panel: the deredened HST light curve and its error in gray. The vertical dot-dashed lines are the beginning and the end of the flares. Bottom panel: the VLA light curve at 13.37 GHz. The vertical dot-dashed line is the time of the change of slope. The dashed broken line is the fit.
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