XMM-Newton light curve of the X-ray from Sgr A* in the 2−10 keV energy range. Left panels: the light curve of flare 1 on 2014 Mar. 10 flare binned on 500 s. Right panels: the light curve of flare 2 on 2014 Apr. 2 flare binned on 100 s. The total (pn+MOS1+MOS2) light curve is shown in the top panel. The light curves of EPIC/pn, MOS1 and MOS2 are shown in the second, third and bottom panels. The crosses are the data points of the total light curve. The horizontal dashed line and the solid line are the sum of the non-flaring level and the smoothed light curve for each instrument. The dashed lines represent the Bayesian blocks. The solid line and the gray curve are the smoothed light curve and the associated errors (h = 500 and 100 s for flare 1 and 2, respectively). The vertical gray stripe is the time during which the camera did not observe.