Top: same as Fig. 1 for HD 134060 b. Bottom: same for the planet’s occultation. The red solid line and blue dashed line show, respectively, models for a central occultation of a 1.85 R_⊕ (Earth-like composition) and 5 R_⊕ (H-dominated composition) planet, assuming a null albedo, an inefficient heat distribution to the night side, and negligible tidal effects for the planet, and assuming black-body emissions for both the planet and its star. The time range of the x-axes of both panels correspond to the same duration so as to outline the fact that the transit timing was much less constrained by the RVs than the occultation timing.