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In this study, ten exoplanets were studied. Their photometric observationswere obtained from the ETD. After performing the data reduction steps, theirparameters were obtained through Exofast online software. Then the total massof the exoplanets and the host stars were obtained through a software that wasmentioned in this study. The location of the host stars in this study was alsoplotted in the H-R diagram.

Estimation of the Total Mass of 10 Exoplanets and their Host Stars Based on the Primary Transit Method