Abstract
BV light curves obtained by Bookmyer (1985) have been analysed with Yamasaki's synthetic technique. As some small difference exists between the light maxima, analysis has been made for the first and the second half of light curve, separately. The result indicates that system parameters deduced from the second half give a better fitting with smaller O-C residuals. These parameters reveal that UZ Pup is contact to the Roche lobe.
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