**Table 7:** Comparison of NGC 2004 analyses in this paper with that from Korn et al. (2000, K00). In K00, NGC 2004-022 is labeled with the Robertson (1974) identification - B30. K00 use LTE model atmospheres with NLTE line formations. Abundances are presented as [X] = 12 + $\log$ ([X/H]) in units of dex.
	NGC 2004-022
	This paper	K00
$T_{\rm eff}$ (K)	21 780	23 450
$\log {g}$ (cm s^-2)	3.15	3.45
$\xi$ (km s^-1)	11	14
C	7.32	7.60:
N	7.68 $\pm$ 0.11	7.50 $\pm$ 0.20
O	8.55 $\pm$ 0.27	8.35 $\pm$ 0.20
Mg	6.94 $\pm$ 0.19	7.00 $\pm$ 0.30
Si	7.23 $\pm$ 0.58	6.90 $\pm$ 0.20
Fe	7.00 $\pm$ 0.22	7.08 $\pm$ 0.30

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