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Table 1

Observing targets.

Name Other Redshifta Systemic Distancea Distancea 12+ Dimensionsa SFR c Logc Logd Log(Total)e
name velocitya (Mpc) method log(O/H)b (arcsec2) (M yr-1) Mstar MHI MHI
(km s-1) (M) (M) (M)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)

CGCG 007-025 0.0048 1449 24.5 CMB 7.74 27.0 × 16.2 0.23 8.36 8.90 8.90
II Zw 40 UGCA 116 0.0026 789 11.7 CMB 8.12 33.6 × 13.2 1.75 8.25 7.54 8.77
Mrk 996 0.0054 1622 18.1 CMB 8.00 36 × 30 0.16 9.18 8.00 8.00
NGC 1140 Mrk 1063 0.0050 1501 19.7 TF 8.18 102 × 54 0.82 9.76 8.56 9.51
NGC 1156 0.0013 375 8.1 Stars 8.23 198 × 150 0.23 9.55 8.66 9.04
NGC 3353 Haro 3, 0.0031 944 18.1 TF 8.37 72.0 × 49.8 1.28 9.54 8.87 8.87
Mrk 35
NGC 7077 Mrk 900 0.0038 1152 17.2 TF 8.03 48 × 42 0.12 8.98 8.15 8.15
SBS 0335052E 0.0135 4043 53.6 CMB 7.25 13.8 × 12.0 1.30 8.51 7.81 8.61
UM 448 Arp 161, 0.0186 5564 81.2 CMB 8.04 24 × 24 11.11 10.91 9.84 9.84
UGC 6665
UM 462 Mrk 1307 0.0035 1057 19.5 CMB 7.97 36 × 30 0.29 8.56 8.30 8.72
UGC 6850

Notes.

(a)

NASA/IPAC Extragalactic Database (NED, http://nedwww.ipac.caltech.edu/): CMB corresponds to Cosmic Microwave Background and TF to Tully-Fisher; velocities are heliocentric; dimensions are optical major and minor diameters.

(b)

Direct-temperature metallicities for CGCG 007025, NGC 3353, UM 448, UM 462, SBS 0335052E from Izotov et al. (2007); II Zw 40 (Thuan & Izotov 2005); Mrk 996 (Thuan et al. 1996); NGC 1140 (Izotov & Thuan 2004); NGC 1156 (Vigroux et al. 1987); NGC 7077 (van Zee & Haynes 2006).

(c)

These quantities are newly derived, as described in Sect. 2.3.

(d)

When these values differ from those in Col. (12), they are calculated from the mean Hi surface density integrated over the optical size of the galaxy.

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