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

Open Access

Fig. B.2

Spectral energy distribution in the range ~0.3−25 µm, used to derive the bolometric luminosity and the stellar radius through the Stefan–Boltzmann equation. The adopted stellar distance is the trigonometric parallax from the Gaia EDR3.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.