Table 5: Abundance uncertainties for a $\Delta T_{\rm eff} = 100$ K, $\Delta$ log g = +0.3, $\Delta v_{\rm t} = 0.2$ km s^-1 and corresponding total error. The errors mean the difference in abundance that needs to be added in order to fit the observed spectrum. The values given are a mean derived from the errors from each line.
Abundance $\Delta T$ $\Delta$ $\log g$ $\Delta v_{\rm t}$ ( $\sum x^{2}$ )^1/2

(100 K) (+0.3 dex) (+0.2 kms^-1)

(1) (2) (3) (4) (5)

HP1-3

[FeI/H] -0.07 -0.07 +0.07 0.12

[O/Fe] +0.00 +0.15 0.00 0.15

[NaI/Fe] +0.03 +0.05 0.00 0.05

[MgI/Fe] +0.01 +0.05 0.00 0.06

[SiI/Fe] -0.09 +0.10 -0.02 0.14

[CaI/Fe] +0.10 +0.10 -0.03 0.15

[TiI/Fe] +0.12 +0.04 -0.01 0.13

[TiII/Fe] -0.01 +0.15 -0.01 0.15

[BaII/Fe] +0.02 +0.05 -0.15 0.16

[LaII/Fe] 0.00 +0.12 0.00 0.12

[EuII/Fe] +0.02 +0.15 0.00 0.15

**Table 5:** Abundance uncertainties for a $\Delta T_{\rm eff} = 100$ K, $\Delta$ log g = +0.3, $\Delta v_{\rm t} = 0.2$ km s^-1 and corresponding total error. The errors mean the difference in abundance that needs to be added in order to fit the observed spectrum. The values given are a mean derived from the errors from each line.
Abundance	$\Delta T$	$\Delta$ $\log g$	$\Delta v_{\rm t}$	( $\sum x^{2}$ )^1/2
	(100 K)	(+0.3 dex)	(+0.2 kms^-1)
(1)	(2)	(3)	(4)	(5)
HP1-3
[FeI/H]	-0.07	-0.07	+0.07	0.12
[O/Fe]	+0.00	+0.15	0.00	0.15
[NaI/Fe]	+0.03	+0.05	0.00	0.05
[MgI/Fe]	+0.01	+0.05	0.00	0.06
[SiI/Fe]	-0.09	+0.10	-0.02	0.14
[CaI/Fe]	+0.10	+0.10	-0.03	0.15
[TiI/Fe]	+0.12	+0.04	-0.01	0.13
[TiII/Fe]	-0.01	+0.15	-0.01	0.15
[BaII/Fe]	+0.02	+0.05	-0.15	0.16
[LaII/Fe]	0.00	+0.12	0.00	0.12
[EuII/Fe]	+0.02	+0.15	0.00	0.15

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