Volume 43 number 2 (2015)
We present new multi-band differential aperture photometry of the eclipsing variable star NSVS 3068865. The light curves are analyzed with the Wilson-Devinney model to determine best-fit stellar models. Our models show that NSVS 3068865 is consistent with a W Ursae Majoris eclipsing variable star near thermal contact with similarities to the aforementioned proto-type.