Table 6: Sensitivities of abundances to variations in the atmospheric parameters.
  $\sigma_{T{\rm eff}}$ $\sigma_{\log g}$ $\sigma_{\xi}$
  $\Delta$: $\pm$70 K $\pm$0.2 dex $\pm$0.15 km s-1
NGC 3960, star c9-310761
${\rm [Fe/H]}$ +0.06/-0.04 +0.01/0.00 -0.05/+0.06
${\rm [Na/Fe]}$ +0.01/-0.02 -0.05/+0.04 +0.02/-0.02
${\rm [Mg/Fe]}$ -0.01/+0.01 -0.01/+0.01 +0.02/-0.02
${\rm [Al/Fe]}$ -0.02/+0.01 -0.02/+0.02 +0.03/-0.03
${\rm [Si/Fe]}$ -0.06/+0.04 +0.02/+0.08 +0.01/-0.03
${\rm [Ca/Fe]}$ +0.01/-0.03 -0.05/+0.03 +0.04/-0.02
${\rm [Ti/Fe]}$ I +0.02/-0.04 -0.03/+0.01 -0.02/+0.01
${\rm [Ti/Fe]}$ II -0.07/+0.06 +0.08/-0.08 -0.03/+0.02
${\rm [Cr/Fe]}$ I +0.01/-0.04 -0.03/+0.00 -0.02/+0.00
${\rm [Cr/Fe]}$ II -0.09/+0.09 +0.08/-0.06 +0.00/-0.01
${\rm [Ni/Fe]}$ -0.02/+0.00 +0.01/-0.02 -0.01/+0.01
${\rm [Ba/Fe]}$ II +0.02/-0.01 +0.04/-0.04 -0.10/+0.08
Berkeley 32, star 17-533
${\rm [Fe/H]}$ +0.06/-0.05 +0.01/0.00 -0.05/+0.06
${\rm [Na/Fe]}$ +0.00/-0.01 -0.03/+0.02 +0.02/-0.02
${\rm [Mg/Fe]}$ -0.05/+0.02 -0.05/-0.02 +0.00/-0.05
${\rm [Al/Fe]}$ -0.02/+0.02 -0.02/+0.01 +0.04/-0.04
${\rm [Si/Fe]}$ -0.06/+0.06 +0.02/-0.03 +0.03/-0.02
${\rm [Ca/Fe]}$ +0.01/-0.03 -0.04/+0.02 -0.01/+0.01
${\rm [Ti/Fe]}$ II -0.08/+0.06 +0.05/-0.11 -0.02/+0.03
${\rm [Ti/Fe]}$ I +0.02/-0.04 -0.02/+0.02 -0.01/+0.01
${\rm [Cr/Fe]}$ I +0.02/-0.03 -0.02/+0.03 -0.01/+0.01
${\rm [Cr/Fe]}$ II -0.10/+0.08 +0.06/-0.11 +0.01/-0.01
${\rm [Ni/Fe]}$ -0.02/+0.01 +0.01/-0.03 +0.00/+0.00
${\rm [Ba/Fe]}$ II +0.02/-0.02 +0.04/-0.05 -0.10/+0.09

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