Fig. 4
Top: 55 Cnc MOST raw photometry with our best-fit global model superimposed. Middle: MOST photometry divided by the best-fit baseline model, and with the best-fit transit + phase-curve model superimposed. Bottom: MOST photometry divided by the best-fit baseline + phase curve model, folded with the best-fit orbital period of 55 Cnc e and binned per 5 min intervals, with the best-fit transit model superimposed.
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