V432 Per
Yang2002 - Yang2002B (Johnson B)
The ephemeris (equation 3) of Yang & Liu (2002) does not phase their light curves well. I remeasured their primary eclipse using both a 2nd degree polynomial and the Kwee Van Woerdan methods and averaged the results for the V-light curve and used their period to obtain the following ephemeris to phase their data: HJD 2450812.0865(4) + 0.38331192E with the probable error of the timing given in parentheses. In their Table 5 of Photometric Solutions their fillout factor is incorrect. To match their radii for the given mass ratio the fillout has to be 0.24, not 0.028 as given. The model with the spot on Star 1 was used for the display.