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Fig. 2


Joint posterior distributions of the central phase and eclipse depth from the 3.6 μm MCMC analysis (left panel), and 4.5 μm (right panel), plotting each point from the MCMC and indicating the density of points by color. The contours (outward to inward) encompass 99%, 10%, and 1% of the points. The crosses mark the best-fit solutions determined by minimal scatter in the Allan deviation relation (see text).

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