Other predictions/data
- Absorption line strengths based on fitting functions
- E-MILES [Na/Fe] enhanced models
- Milky Way Globular Clusters high-resolution integrated spectroscopic data
- E-MILES models with ages <63 Myr
- Surface Brightness Fluctuation spectra from the extended MILES
- sMILES: Semi-Empirical MILES Stellar Spectral Library, with varying [α/Fe]
- sMILES: Semi-Empirical MILES Stellar Population Models with Variable [α/Fe] Abundances