The goal here is to add simple binaries to the stellar models. These would be physical binaries having the same metallicity and age. The parameter space could be/should be reduced further by only including binaries that produce SEDs in the target bands that are detectably different than single stars (e.g., the most luminous of the two).
The goal here is to add simple binaries to the stellar models. These would be physical binaries having the same metallicity and age. The parameter space could be/should be reduced further by only including binaries that produce SEDs in the target bands that are detectably different than single stars (e.g., the most luminous of the two).