Table 1.
Properties of our target galaxies.
| Galaxy | DM | Distance | AV | Z | Lref1 |
|---|---|---|---|---|---|
| [mag] | [Mpc] | [mag] | [Z⊙] | ||
| I Zw 18 | 31.3 a) | 18.2 | 0.1 b) | 1/40 c) | TW |
| SMC | 18.977 d) | 0.062 | 0.35 e) | 1/5 f) | g), TW |
| NGC 5253 | 27.48 h) | 3.1 | 0.3 i) | 1/3 j) | TW |
| NGC 300 | 27.36 k) | 3.0 | 0.15 l) | 1/2.5 m) | TW |
| LMC | 18.476 n) | 0.050 | (not used) | 1/2 o) | g) |
| NGC 4395 | 28.15 p) | 4.3 | 0.3 q) | 1 r) | TW |
| M 31 | 24.407s) | 0.761 | (not used) | 1.5t) | u) |
Notes. 1: Lref refers to the work (i.e., TW) in which cool SG luminosities were measured. References: a): Aloisi et al. (2007) – b): Izotov & Thuan (2016), Hirschauer et al. (2024) – c): from Lebouteiller et al. (2013) and from oxygen abundances of Skillman & Kennicutt (1993) compared to log(O/H)⊙ = 8.75 (Bergemann et al. 2021) – d): Graczyk et al. (2020) – e): Schootemeijer et al. (2021) – f): Venn (1999) – g): Davies et al. (2018) – h): Davidge (2007) – i): Abril-Melgarejo et al. (2024) – j): Monreal-Ibero et al. (2012) – k): Rizzi et al. (2006) – l)Micheva et al. (2022) – m): Gazak et al. (2015) – n): Pietrzyński et al. (2019) – o): Davies et al. (2015), Patrick et al. (2016), Choudhury et al. (2021) – p): Thim et al. (2004) – q): based on A263 nm ≈ 0.75 (Nandi et al. 2023) and Aλ/AV from Gordon et al. (2003) – r): Cedrés & Cepa (2002) – s): Li et al. (2021) – t): based on Zaritsky et al. (1994) and Bergemann et al. (2021) – u): McDonald et al. (2022).
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