Table 1
Properties of target galaxies.
| Galaxy | RA | Dec | d | Z(a) | R |
|---|---|---|---|---|---|
| Galaxy | (J2000) | (J2000) | (Mpc) | (Z⊙) | (′) |
| WLM | 00:01:58.16 | −15:27:39.3 | 0.96 ± 0.05 | 0.14(1) | 9 |
| NGC 55 | 00:14:53.60 | −39:11:47.9 | 1.99 ± 0.06 | 0.27(2) | 21 |
| NGC 247 | 00:47:08.55 | −20:45:37.4 | 3.52 ± 0.06 | 0.40(3) | 14 |
| NGC 253 | 00:47:33.12 | −25:17:17.6 | 3.56 ± 0.08 | 0.72(4) | 21 |
| NGC 300 | 00:54:53.48 | −37:41:03.8 | 1.98 ± 0.06 | 0.41(5) | 15 |
| NGC 1313 | 03:18:16.05 | −66:29:53.7 | 4.25 ± 0.08 | 0.35(6) | 8 |
| NGC 3109 | 10:03:06.88 | −26:09:34.5 | 1.37 ± 0.06 | 0.21(7) | 13 |
| Sextans A | 10:11:00.80 | −04:41:34.0 | 1.37 ± 0.06 | 0.06(8) | 4 |
| M83 | 13:37:00.95 | −29:51:55.5 | 4.66 ± 0.07 | 1.58(9) | 10 |
| NGC 7793 | 23:57:49.83 | −32:35:27.7 | 3.58 ± 0.07 | 0.42(10) | 8 |
Notes. (a)Metallicities are based on young clusters or massive stars, when available. An average value was reported in cases where multiple measurements or radial gradients exist.
References. (1) Urbaneja et al. (2008); (2) Hartoog et al. (2012); (3) Davidge (2021); (4) Spinoglio et al. (2022); (5) Kudritzki et al. (2008); (6) Hadfield & Crowther (2007); (7) Hosek et al. (2014); (8) Kniazev et al. (2005); (9) Hernandez et al. (2019); (10) Della Bruna et al. (2021).
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