A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO - Radial velocities lead to the detection of transits with low signal-to-noise ratio

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Fig. B.4

Corner plots showing the posteriors of the free parameters adopted for the planetary internal structure modelling described in Sect. 6. From top to bottom, the plots refer to HIP 29442 b, HIP 29442 c, and HIP 29442 d.

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