Table 1: Available stellar isochrones including the TP-AGB phase.

Reference	DU and HBBa	b	Dustc	Public www address for retrieval
Bertelli et al. (1994), A&AS, 106, 275	NO	solar-scaled comp.	NO	http://pleiadi.pd.astro.it
Bressan et al. (1998), A&A, 332, 135	NO	solar scaled comp.	YES	upon request
Girardi et al. (2000), A&AS, 141, 371	NO	solar-scaled comp.	NO	http://pleiadi.pd.astro.it
Marigo & Girardi (2001), A&A, 377, 132	YES	solar-scaled comp.	NO	http://pleiadi.pd.astro.it
Mouhcine (2002), A&A, 394, 125	YES	solar scaled comp.	YES	upon request
Piovan et al. (2003), A&A, 408, 559	NO	solar scaled comp.	YES	upon request
Marigo et al. (2003a), A&A, 403, 225	YES	O-/C-rich comp.	NO	upon request
Cioni et al. (2006), A&A, 448, 77	YES	O-/C-rich comp.	NO	http://pleiadi.pd.astro.it
Cordier et al. (2007), AJ, 133,468	NO	solar scaled comp.	NO	http://www.oa-teramo.inaf.it/BASTI
This work	YES	O-/C-rich comp.	YES	http://stev.oapd.inaf.it/cmd

a Explicit inclusion or not of AGB nucleosynthesis, i.e. the third dredge-up and hot-bottom burning, in the underlying AGB models. b Choice of low-temperature opacities affecting the predicted effective temperature, i.e. for solar-scaled or variable (O- or C-rich) chemical mixtures. c Inclusion or not of circumstellar dust in the computation of the emitted spectrum.

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