Table 4: Comparison of bump properties for stellar models of $1~M_\odot$ and Z=0.001. The references are: Girardi et al. (2000, Padova), Cariulo et al. (2004, Pisa), Pietrinferni et al. (2004, BASTI), and Kim et al. (2002, Y2).
  Padova Pisa BASTI Y2 This work
Age (Gyr) 6.514 6.331 6.023 6.769 6.222
$\log L/L_\odot$ 1.971 2.089 2.106 2.101 2.153
$\log T_{\rm eff}$ 3.698 3.689 3.694 3.689 3.693
Metal mix. solar solar $\alpha$-enh. $\alpha$-enh. $\alpha$-enh.
Diffusion no yes no yes yes

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