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Table 5

The sensitivity to [Fe/H], [Ba/H], νconv and fodd for different values of Teff and log g.

f odd
Teff (K) log g (cgs) νconv (kms-1) [Fe/H] [Ba/H] 4554 Å 4934 Å
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
case 1 case 2 case 1 case 2 case 1 case 2 case 1 case 2 case 1 case 2
5500 3.4 5.79 ...  −2.78 ...  −3.69  −3.71  −0.01 0.02 0.15  −0.115
5500 3.7 5.67 ...  −2.77 ...  −3.59  −3.61 0.05  −0.01 0.20  −0.115
5500 4.0 5.52 ...  −2.74 ...  −3.50  −3.50 0.11  −0.07 0.24  −0.111
5750 3.4 5.82 ...  −2.60 ...  −3.50  −3.52  −0.02 0.04 0.09 0.113
5750 3.7 5.75 5.75  −2.59  −2.59  −3.42  −3.42 0.01 0.01 0.11 0.112
5750 4.0 5.60 ...  −2.57 ...  −3.33  −3.31 0.09  −0.03 0.15 0.112
6000 3.4 5.84 ...  −2.43 ...  −3.34  −3.34  −0.03 0.04 0.02 0.252
6000 3.7 5.77 ...  −2.42 ...  −3.24  −3.24 0.01 0.02 0.04 0.252
6000 4.0 5.69 ...  −2.40 ...  −3.15  −3.14 0.04 0.00 0.05 0.245

Notes. Case 1: the sensitivity of all atmospheric parameters used or calculated in this analysis to changes in temperature and log g. Case 2: the sensitivity of [Ba/Fe] and fodd to temperature and log g. Macroturbulence and [Fe/H] are fixed to values found for the model atmosphere used in this analysis (Teff = 5750, log g = 3.7, νconv = 5.75   kms-1,  [Fe/H]  =  −2.59). Columns (11) and (12) show the sensitivity of the blended 4934 Å line to changes in the stellar parameters.

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