I have completed all of the new lens flares except for δ Serpentis. I have the lens flares for the subgiant twins A and B, however, I do not know the spectral classes of the distant pair C and D. I have checked catalogs of multiple and optical stars and the data is not available. I guess I am striving too hard for "realism". If necessary, we can just assume that the distant pair is of the same spectral class as the primary pair of stars. Anyway, if that's fine then I guess I am done with the lens flares. The RGB values are as follows:
α Orionis: Same
β Aquilae A: 255 225 189
β Aquilae B: Same
β Aquilae C: Same
δ Serpentis A: Same
δ Serpentis B: Same
δ Serpentis C: 218 224 255
δ Serpentis D: 218 224 255
If this is fine, I'll hand over the flares tomorrow. As for Laramis, if a star is needed for the system just let me know the specifics and requirements and I'll make it. δ Trianguli would make a great system. I think close binaries of all types are just awesome, so I'll add this system to my list.