Open Access

Fig. 4

image

Download original image

Analysis of the rotation period of TOI-1430 performed with different photometric series. The left panels show the light curves folded with the period associated with the peak of the corresponding GLS periodogram (right panels). Φ is the rotational phase of the star. From the upper panel to the bottom, we report the analysis carried out on TESS, KELT, STELLA, and Asiago Schmidt light curves, respectively.

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.