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The flux distribution of Sgr A*

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Figure

Fig. 1. Binary fit to interferometric quantities for the night of July 28, 2018. The three panels show the best-fit binary model to the visibility modulus, the visibility squared, and the closure phase.
Fig. 2. Light curve of Sgr A* as observed by GRAVITY in the years 2017, 2018, and 2019 with time gaps removed.
Fig. 4. SED of Sgr A*: the radio and sub-mm data are from Falcke et al. (1998), Bower et al
Fig. 5. Distribution fits: the observed flux distribution is fitted with a lognormal PDF
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