Table 8: Abundances and NIR luminosities for the fiducial sample of galaxies. Distances are expressed in Mpc, and Cols. 6 and 7 indicate the method used to compute the distance, and its reference. Our abundances have been corrected by -0.1 dex. For comparison we add also I Zw 18 (H=16.03 $\pm $ 0.15; Thuan 1983) and SBS 0335-052 (H=16.09 $\pm $ 0.03, $15\hbox {$^{\prime \prime }$ }$ aperture; Vanzi et al. 2000).
Galaxy Group $12+\log{\rm (O/H)}$ Ref. Distance Met. Ref. MH
ESO 347-G017 Scl $7.90\pm0.05$ S08#1 $6.99\pm1.40$ J98 S03a $-17.40\pm0.66$
NGC 59 Scl $8.29\pm0.08$ S08#1 $4.39\pm0.87$ J98 S03a $-17.97\pm0.57$
ESO 473-G024 Scl $7.49\pm0.06$ S08 $5.94\pm1.19$ J98 S03a $-14.85\pm0.92$
NGC 625 Scl $8.27\pm0.06$ S08#2 $3.89\pm0.22$ RGBT C03 $-18.95\pm0.28$
ESO 245-G005 Scl $8.07\pm0.21$ S08c $4.43\pm0.45$ RGBT K03 $-17.24\pm0.54$
UGC 4483 M 81 $7.51\pm0.08$ S08 $3.40\pm0.20$ RGBT IT02 $-13.99\pm0.57$
UGCA 442 M 81 $7.72\pm0.03$ S03b $4.27\pm0.52$ RGBT K03 $-16.45\pm0.56$
DDO 42 M 81 $7.90\pm0.01$ I97 $3.20\pm0.41$ RGBT K02 $-17.40\pm1.03$
I ZW 18 - SE ... $7.26\pm0.05$ SK03 $18.2\pm1.5$ RGBT A08 $-15.27\pm0.23$
I ZW 18 - NW ... $7.17\pm0.04$ SK03 $19.3\pm2.3$ Ceph. A08 $-15.40\pm0.28$
SBS 0335-052 ... $7.29\pm0.02$ I06 $54.8\pm3.8$ Hub.fl. NED $-17.60\pm0.15$

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