Table 14: NGC 3960: comparison with the results by Bragaglia et al. (2006a); numbers in parenthesis are their IDs.
star   $T_{\rm eff}$ log g $\xi$ [Fe/H] $\Delta{\log n(\rm {Fe})}$
    K   km s-1    
c5 MOOG 4870 2.16 1.22 +0.00 -0.09
(41) ROSA 4850 2.20 1.21 -0.14  
c6 MOOG 4950 2.40 1.19 +0.02 -0.12
(28) ROSA 4900 2.06 1.23 -0.15  
c8 MOOG 5040 2.57 1.17 +0.00 -0.01
(50) ROSA 5000 2.70 1.15 -0.06  

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