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Fig. 11

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Spitzer photometry divided by the best-fit baseline model and binned per 0.005d = 7.2 min, with the best-fit transit model overplotted in red. Below are shown the y-shifted residuals of the fit binned per 7.2 min and 30 min intervals. Their standard deviations are, respectively, 57 ppm and 25 ppm. Over the light curve is shown the prior probability distribution function derived for the transit timing of HD 219134 b from our analysis of the HARPS-N RVs.

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