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WASP-64b and WASP-72b: two new transiting highly irradiated giant planets

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Academic year: 2021

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Figure

Table 1. Summary of follow-up photometry obtained for WASP-64 and WASP-72. N= number of measurements
Fig. 4. Follow-up transit photometry for WASP-64 b. For each light curve, the best-fit transit+baseline model deduced from the global analysis is superimposed (see Sec
Fig. 6. Follow-up transit photometry for WASP-72 b. For each light curve, the best-fit transit+baseline model deduced from the global analysis is superimposed (see Sec
Fig. 8. T op: CORALIE RVs for WASP-72 phase-folded on the best-fit orbital period, and with the best-fit Keplerian model over-imposed
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