Narrow-band indices for simple stellar population models. The models include the original 21 indices of the Lick-IDS system (Worthey et al. 1994, ApJS, 94, 687) + 4 additional higher-order Balmer lines (Worthey & Ottaviani 1997, ApJS, 111, 377) + Near InfraRed indices from Cenarro et al. (2001, MNRAS, 326, 959).
The SSps are based on
- Bertelli et al. 1994 isochrones (A&ASS, 106, 275)
- Spectral libraries originally adopted by Bressan et al. (1994, ApJS, 94, 63)
and revised by Tantalo et al. 1996 (A&A, 311, 361)
- Fitting Functions of Worthey et al. 1994 (ApJS, 94, 687),
Worthey & Ottaviani 1997 (ApJS, 111, 377) and
Cenarro et al. 2002 (MNRAS, 329, 863)
Download SPPs tables
References
Annibali et al. 2007, A&A, 463, 455