  BW Aqr is a bright eclipsing binary star containing a pair of F7V stars. The
absolute parameters of this binary (masses, radii, etc.) are known to good
precision so they are often used to test stellar models, particularly in
studies of convective overshooting. ... Maxted & Hutcheon (2018) analysed the
Kepler K2 data for BW Aqr and noted that it shows variability between the
eclipses that may be caused by tidally induced pulsations. ... Table 1 shows
the absolute parameters for BW Aqr derived from an improved analysis of the
Kepler K2 light curve plus the RV measurements from both Imbert (1979) and
Lester & Gies (2018). ... The values in Table 1 with their robust error
estimates from the standard deviation of the mean are consistent with the
values and errors from Maxted & Hutcheon (2018) based on the PPD calculated
using emcee for a fit to the entire K2 light curve.
