Fig. 3
Overshoot of the transit depth as a function of the limb darkening parameters a and b in the case of quadratic limb darkening via Eq. (3). For this plot, a transit impact parameter p = 0 has been chosen. The positions of several main-sequence stars as per Claret & Bloemen (2011) are indicated with filled circles in the a–b plane (see Table 1).
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