Ratios of limb-transit spectra to out-of-transit spectra for stars with different Teff. These spectra are simulated using the planetary and stellar parameters described in Sect. 5.1. Here, the limb-transit is defined as the orbital phase with the deepest line depth measured by using a 1.5 Å band centred at the D2 line. This figure presents the change of the CLV effect with Teff.
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