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Fig. 5


Comparing the best fit model to the transit photometry of HAT-P-11 using SOAP-T and the Kepler observation of HAT-P-11 for one period of stellar rotation. Red (dash-dotted) line shows SOAP-T’s photometric result for an edge-on solution and green (dashed) line correspond to HAT-P-11 observation. The blue (solid) line in the bottom panel shows the residual.

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