Best light curve fit for PHOEBE model 1 of eclipsing binary assuming primary has mass consistent with K5V star, and secondary is massive enough to burn hydrogen (i = 44°, q = 0.11, M1 = 0.73 M⊙, M2 = 0.08 M⊙). Binned input SuperWASP light curve shown with diamonds and uncertainty bars; fit with dotted line.
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.