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Table A.1.

Numbers of certain types of stars and SFRs in different galaxies.

Galaxy SFR (lit.) NHeB,  lit. SFR NcSG,  obs SFRmin NcSG,  pred NcSG,  obs NWR,  obs
[M yr−1] (5< logL< 5.6) (5< logL< 5.6) [M yr−1] (logL> 5.6) (logL> 5.6) (logL> 5.6)
I Zw 18 0.1-1 150-1500 28 0.019 90 (10a)) 0 "tens" (estimated, no L provided)
SMC 0.05 75 41b) 0.027 32 0 11 (3 can be H-burningc))
NGC 5253 0.1, 0.2 150, 300 71 0.047 52 1 30 to 40 (estimated, no L provided)
LMC 0.2 300 72b) 0.048 21 1 ∼80 (half can be H-burningc))
NGC 300 0.08-0.16 120-240 86 0.057 21 0 30 to 40 (estimated, no L provided)
NGC 4395 0.03, 0.5 45, 750 86 0.057 19 0 "WR features"
M 31 0.7 1050 117d) 0.078

Notes. The text in Appendix A.1 describes how numbers of cool SG stars and the minimum SFRs are obtained. Explanation of notes in the table: a): if, instead, a constant cool SG lifetime fraction of 7% of the stellar lifetime is assumed – b): from Davies et al. (2018)c): these stars can be hydrogen burning because they have temperatures lower than the zero-age main-sequence temperature. – d): from McDonald et al. (2022). Literature SFR references are the following. I Zw 18: table 1 of Hirschauer et al. (2024), Bortolini et al. (2024); SMC: Harris & Zaritsky (2004); N5253: López-Sánchez et al. (2012); LMC: Harris & Zaritsky (2009); N300: Helou et al. (2004), Kang et al. (2025); N4395: Smirnova et al. (2020), Nandi et al. (2023); M31: Lewis et al. (2015). References for NWR,  obs: Sect. 5.3.4, and Hainich et al. (2014, 2015) for LMC and SMC, respectively.

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