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Fig. 8


Light curve of HD 189733 as observed by the LPC camera during 2016Q3. The data have been phase-folded to the orbital period of HD 189733 b. Panel a: light curve after primary calibration, with the median subtracted for clarity. Panels b–d: light curve for each of the secondary calibration methods, Fourier, Legendre and Local Linear respectively. The RMS scatter on the light curve is noted in the top-right of each panel.

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