Table A.1: MILES to Lick/IDS transformation.
Index Slope (m) Intercept (q) rms
H$\beta $ 0.97 0.12 0.27
Mgb 0.88 0.31 0.41
Fe5270 0.91 0.16 0.32
Fe5335 0.94 0.23 0.34
H $\gamma_{\rm A}$ 0.95 -0.30 0.80
H $\delta_{\rm A}$ 0.94 -0.17 0.85
H $\gamma_{\rm F}$ 0.96 -0.15 0.46
H $\delta_{\rm F}$ 0.95 0.02 0.49
The calibrated index is $i_{\rm Lick/IDS}=m\times{i_{\rm MILES}}+q$; the rms is calculated on the basis of $\sim $240 stellar spectra.

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