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Using a huge library of 1-Å resolution spectra over a wide range of log T eff , log g and [Fe/H] and for both solar and α-enhanced abundance ratios [α/Fe], we present theoretical absorption-line indices in the Lick system. First we derive the response functions (RF s) for a wide range of log T eff , log g, [Fe/H], and [α/Fe] = +0.4 dex. The RF s are commonly used to correct indices with solar [α/Fe] ratios to indices with [α/Fe] > 0. The RF s vary not only with the type of star but also withdoi:10.1017/s174392130700765x fatcat:dbyn47qc4fd5jpxj3twzv5taom