Open Access

Fig. 3.


Doppler data time-series of HD 23472 obtained with HARPS. The small number of data points (14) by itself is not sufficient to discover the planets, but taking advantage of the a priory knowledge of the TESS transit ephemerids, it enables constructing a two-planet model, which is in excellent agreement with the RV data (see Table 2 for details). As in Fig. 2, the RV uncertainties include the RV jitter.

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.