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Fig. D.2.

image

Light curves with a time bin of 2.5 s as observed by Swift during the first two observations in 2016 that were tagged as flares. The black lines show the Sgr A* count rate and the red lines represent the average light curve of the PSF tail of the two transients at the same distance as Sgr A*. The vertical bars are the 1σ error bars.

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