Digging deeper into the dense Galactic globular cluster Terzan 5 with electron-multiplying CCDs - Variable star detection and new discoveries

Open Access

Fig. 14

Light curve of variable star G10. The top panel shows the light curve in I magnitude versus HJD while the bottom panel shows the phased light curve with the periods and epochs given in Table A.1. Colours are the same as in Fig. 1.

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.