Fig. 8.

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Data and plasmoid models of the flares from July 22, 2018. The left panels shows the astrometry of the flare while the right panel shows the observed (full line) and intrinsic (dashed line) light curves. The parameters of the model are listed in Tables 3 and 4. Note that this is not the result of a fit. The black dot in the left panels represents the position of Sgr A* in GYOTO and the orange cross represent the position of Sgr A* measured through the orbit of S2.
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