Currently what I am attempting to do is to generate a spectrum from FERRE that represents a binary system and see how well it fits the observed spectrum.

So far I’ve generated the spectra of the two stars and shifting them by using the velocities generated by martins SB2 code.

The next step is now fitting the the model spectra of the individual stars with the observed spectra.

To do this I will create a “model temperature grid” holding a range that will be tested against the observed spectra and continue to narrow that range until we have a proper approximation.