TESS search for substellar companions through pulsation timing of δ Scuti stars - I. Discovery of companions around Chang 134 and V393 Car

Open Access

Fig. 5

Linear orbital solution for V393 Car. Upper panel: same as Fig. 4, but with the best-fit LTTE solution with a linear baseline (O–C)_lin (Eq. (8)). The linear baseline a₀ + a₁t is plotted separately as a dashed orange line. Lower panel: residuals from the best-fit model in seconds.

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.