First Photometric Observations of Recently Discovered Binaries

We present preliminary results of BVRI photometry of binary stars out of an observing list of short period binaries without any previous multifilter observations. The purpose of this project is to obtain photometric elements and the absolute parameters for further understanding of the evolutionary processes for these systems. The observations took place at the Kryonerion Astronomical Station (NOA). New times of minima are presented and a more accurate ephemeris is suggested.