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Fig. 4.

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Transit of HD 189733 b observed by TESS with a cadence of 120 s. Black dots represent the mean of consecutive subsets of ten observations. Maximum likelihood fits from the nDR = 1 and nDR = 0 models are marked with orange and blue lines respectively, one sigma uncertainties are marked as shaded areas. The residuals of the highest likelihood nDR = 1 and nDR = 0 model fits are shown in the middle and the bottom of the figure, respectively. The feature between t − tc ≈ −2200 s and t − tc ≈ −300 s is an eclipse of a dark region with a radius of r min = 9 . 8 2.2 + 4.5 $ r_{\mathrm{min}} = 9.8_{-2.2}^{+4.5} $ ° and a contrast of 0.04.

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