Fig. G.1.

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Flare models for a hot spot ejection velocity of 0.1c and foot-point orbital velocities between 0.8uK and 0.9uK (red lines) overlapped with the observations of July 22, 2018 (gray circles). The direction of motion is indicated by blue arrows. The position of SgrA* in the sky is denoted by a black cross, and the best-fit black hole position, which is slightly different for each model, by a blue rectangle.
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