Fig. 4
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Fitting the phase curve and transit of a deformed planet with a spherical planet model. Left: simulated deformed planet phase curve of WASP-12 b in the TESS (blue) and NIRSpec-PRISM (red) bands. The spherical planet model fit is overplotted for each light curve. The bottom panel shows the residuals of the fit for each light curve. Right: same as the left panel, but for observation of the transit only. The residuals are shown in the bottom panel for each light curve with the root sum of squares (RSS) quoted.
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