Open Access

Fig. 12

image

Transit spectra for 100×, 300× and 1000× solar metallicity, for cloud-free cases (solid red lines), fully cloudy cases (dotted red lines), and with partial cloud cover (blue regions). The simulations were performed with 106 CCN kg−1 for the bottom left panel and with 105 CCN kg−1 for the other panels. K2 and HST data from Benneke et al. (2019b) are indicated with black dots.

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