Table 1.
Properties of the program galaxies.
| Name | DDO | Distance | Distance modulus | Radial velocity | [Fe/H] | SFR ( † ) |
|---|---|---|---|---|---|---|
| identifier | (kpc) | (mag) | (km s−1) | (dex) | M⊙ yr−1 | |
| IC 10 | 794±44 | 24.27±0.18 | −348 ±1 | −0.50 (a) | 0.05 (b) | |
| IC 1613 | DDO 8 | 755±42 | 24.39±0.12 | −233 ±1 | −0.67 (h) | 0.0029 (c) |
| Pegasus | DDO 216 | 920±30 | 24.82±0.07 | −183 ±5 | −0.80 (a) | 0.00035 (d) |
| Phoenix | 415±19 | 23.09±0.10 | −13 ±9, −52±6 (j) | – | – | |
| Sextans A | DDO 75 | 1432±53 | 25.60±0.03 | +324 ±2 | −1.0 (i) | 0.002 |
| Sextans B | DDO 70 | 1426±20 | 25.60±0.03 | +304 ±1 | – | 0.002 (e), (0.0008) |
| WLM | DDO 221 | 933±34 | 24.95±0.03 | −130 ±1 | −0.87 (f) | 0.00047 (g), (0.003) ( * ) |
Notes. ( * )The distance, distance moduli, systemic radial velocities, and metallicities are taken from McConnachie (2012). ( † )Star formation rates are taken from Mateo (1998).
References.(a) Bergh (2000), (b) Yin et al. (2010), (c) Cole et al. (1999), (d) Gallagher et al. (1998), (e) Tosi et al. (1991), (f) Urbaneja et al. (2008), (g) Tosi et al. (1989), (h) Tautvaišienė et al. (2007), (i) Kaufer et al. (2004), (j) Gallart et al. (2001).
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