Estimate physical quantities of a binary star system from observed quantities.
The purpose of this project is to estimate physical quantities of an eclipsing, spectroscopic binary star system using observed quantities from photometry and spectroscopy. The estimated physical quantities serve as input to a more complete numerical model such as that of Wilson-Devinney, c.f. chapter 7 of . The model used in this project is a simple, spherical detached binary star model with no orbital eccentricity and no limb darkening. The model is from chapter 7 of  and chapter 7 of .