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Table E.1.

Summary of the observational data used in this study.

Object redshift log10(sSFR/yr) [O/Fe] systematics ZFe method reference comment
Milky Way 0 -10.4 0.19 + 0.2 $ ^{+0.2}_{-0.19} $ -0.36 0.27 + 0.27 $ ^{+0.27}_{-0.27} $ +ADF, +Δd young clusters [1, 2, 3, 4] Rgal = 8 kpc
Milky Way 0 -10.4 0.19 + 0.2 $ ^{+0.2}_{-0.19} $ -0.4 0.25 + 0.25 $ ^{+0.25}_{-0.25} $ +ADF, +Δd young clusters [1, 2, 3, 4] Rgal = 6.8 kpc
LMC 0 -9.7 0.3 + 0.3 $ ^{+0.3}_{-0.3} $ -0.15 0.23 + 0.23 $ ^{+0.23}_{-0.23} $ +ADF, +Δd stellar spectra [5, 6, 7]
SMC 0 -10.1 0.3 + 0.3 $ ^{+0.3}_{-0.3} $ -0.17 0.12 + 0.12 $ ^{+0.12}_{-0.12} $ +ADF, +Δd stellar spectra [5, 6, 7]
IZw18 0 -7.56 0.03 + 0.04 $ ^{+0.04}_{-0.03} $ 0.25 0.05 + 0.05 $ ^{+0.05}_{-0.05} $ ICF, Fe HII region [8, 8, 9]
Sextans A 0 -9.87 0.4 + 0.33 $ ^{+0.33}_{-0.4} $ -0.2 0.25 + 0.25 $ ^{+0.25}_{-0.25} $ +ADF, +Δd stellar spectra [10, 11, 12, 13]
NGC 3109 0 -9.83 0.17 + 0.17 $ ^{+0.17}_{-0.17} $ -0.39 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ +ADF, +Δd BSG [14, 15, 13]
- 3.4 -7.63 0.1 + 0.12 $ ^{+0.12}_{-0.1} $ -0.0038 0.059 + 0.059 $ ^{+0.059}_{-0.059} $ +ADF, +Δd, +ΔSPS UV cont., S99 [16]
- 3.4 -7.54 0.02 + 0.07 $ ^{+0.07}_{-0.02} $ 0.021 0.059 + 0.059 $ ^{+0.059}_{-0.059} $ +ADF, +Δd, +ΔSPS UV cont., S99 [16]
- 3.4 -7.55 0.03 + 0.15 $ ^{+0.15}_{-0.03} $ 0.14 0.054 + 0.054 $ ^{+0.054}_{-0.054} $ +ADF, +Δd, +ΔSPS UV cont., S99 [16]
- 3.2 -7.62 0.09 + 0.05 $ ^{+0.05}_{-0.09} $ 0.34 0.046 + 0.046 $ ^{+0.046}_{-0.046} $ +ADF, +Δd, +ΔSPS UV cont., S99 [16]
high M* stack 3.4 -8.31 0.5 + 0.5 $ ^{+0.5}_{-0.5} $ 0.28 0.023 + 0.023 $ ^{+0.023}_{-0.023} $ +ADF, +Δd, +ΔSPS UV cont., S99 [16] stack, ΔSPS = 0.04
low M* stack 3.4 -7.79 0.42 + 0.42 $ ^{+0.42}_{-0.42} $ 0.21 0.013 + 0.013 $ ^{+0.013}_{-0.013} $ +ADF, +Δd, +ΔSPS UV cont., S99 [16] stack, ΔSPS = 0.6
KBSS-LM1 stack 2.4 -8.43 0.33 + 0.33 $ ^{+0.33}_{-0.33} $ 0.46 0.076 + 0.076 $ ^{+0.076}_{-0.076} $ -ADF, +Δd UV cont., BPASS/S99 [17] stack
high stack 2.3 -9.17 0.6 + 0.6 $ ^{+0.6}_{-0.6} $ 0.34 0.12 + 0.085 $ ^{+0.085}_{-0.12} $ -ADF, +Δd, -ΔSPS UV cont., BPASS [18] stack
low stack 2.3 -8.74 0.47 + 0.47 $ ^{+0.47}_{-0.47} $ 0.72 0.13 + 0.21 $ ^{+0.21}_{-0.13} $ -ADF, +Δd, -ΔSPS UV cont., BPASS [18] stack
J1142-0038 0.02 -6.02 0 + 0.03 $ ^{+0.03}_{-0} $ 0.79 ICF, Fe HII region [19] lower limit
J1429-0110 0.03 -6.12 0.08 + 0.12 $ ^{+0.12}_{-0.08} $ 0.66 0.075 + 0.091 $ ^{+0.091}_{-0.075} $ ICF, Fe HII region [19]
J1631+4426 0.031 -7.17 0.08 + 0.09 $ ^{+0.09}_{-0.08} $ -0.24 0.12 + 0.12 $ ^{+0.12}_{-0.12} $ ICF, Fe HII region [19, 21, 19]
J0002+1715 0.021 -7.06 0.02 + 0.02 $ ^{+0.02}_{-0.02} $ 0.8 0.027 + 0.035 $ ^{+0.035}_{-0.027} $ ICF, Fe HII region [19]
J1642+2233 0.017 -6.23 0.12 + 0.02 $ ^{+0.02}_{-0.12} $ 1 0.038 + 0.027 $ ^{+0.027}_{-0.038} $ ICF, Fe HII region [19]
J2115-1734 0.023 -6.29 0.01 + 0.01 $ ^{+0.01}_{-0.01} $ 0.31 0.026 + 0.026 $ ^{+0.026}_{-0.026} $ ICF, Fe HII region [19]
J2253+1116 0.0073 -6.32 0 + 0 $ ^{+0}_{-0} $ 0.75 0.022 + 0.02 $ ^{+0.02}_{-0.022} $ ICF, Fe HII region [19]
J2310-0211 0.012 -7.15 0.02 + 0.02 $ ^{+0.02}_{-0.02} $ 0.72 0.023 + 0.019 $ ^{+0.019}_{-0.023} $ ICF, Fe HII region [19]
J2327-0200 0.018 -6.69 0.02 + 0.01 $ ^{+0.01}_{-0.02} $ 0.56 0.017 + 0.022 $ ^{+0.022}_{-0.017} $ ICF, Fe HII region [19]
J0811+4730 0.044 -6.56 0.31 + 0.31 $ ^{+0.31}_{-0.31} $ -0.27 0.092 + 0.092 $ ^{+0.092}_{-0.092} $ ICF, Fe HII region [20]
J082555 0.0024 -8.11 0 + 0 $ ^{+0}_{-0} $ 0.34 0.2 + 0.15 $ ^{+0.15}_{-0.2} $ -ADF, -Δd, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $ UV cont. S99/C&B [22, 22, 23] [O/Fe] using S99 SPS, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $= 0 + 0.24 $ ^{+0.24}_{-0} $
J104457 0.013 -7.82 0 + 0 $ ^{+0}_{-0} $ 0.35 0.2 + 0.17 $ ^{+0.17}_{-0.2} $ -ADF, -Δd, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $ UV cont. S99/C&B [22, 22, 23] [O/Fe] using S99 SPS, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $= 0.0076 + 0.1 $ ^{+0.1}_{-0.0076} $
HS1442+4250 0.0022 -7.75 0.28 + 0.28 $ ^{+0.28}_{-0.28} $ 0.69 0.098 + 0.072 $ ^{+0.072}_{-0.098} $ -ADF, -Δd, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $ UV cont. S99/C&B [22, 22, 24] [O/Fe] using S99 SPS, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $= 0.37 + 0.1 $ ^{+0.1}_{-0.37} $
SB2 0.0049 -6.98 0.04 + 0.04 $ ^{+0.04}_{-0.04} $ 0.63 0.22 + 0.2 $ ^{+0.2}_{-0.22} $ -ADF, -Δd, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $ UV cont. S99/C&B [22, 22, 25] [O/Fe] using S99 SPS, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $= 0.18 + 0.1 $ ^{+0.1}_{-0.18} $
SB82 0.017 -6.98 0.16 + 0.16 $ ^{+0.16}_{-0.16} $ 0.73 0.16 + 0.17 $ ^{+0.17}_{-0.16} $ -ADF, -Δd, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $ UV cont. S99/C&B [22, 22, 25] [O/Fe] using S99 SPS, Δ SPS $ \Delta_{\mathrm{SPS}}^{*} $= 0.097 + 0.1 $ ^{+0.1}_{-0.097} $
- 2.3 -8.62 0.28 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ HII region/indirect [26] median
- 2.3 -8.62 0.25 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ d HII region/indirect [27] median
AEGIS_11452 1.7 -8.25 0.38 + 0.08 $ ^{+0.08}_{-0.38} $ -0.13 2.4 + 0.53 $ ^{+0.53}_{-2.4} $ -ADF, +Δd HII region/indirect [28]
COSMOS_1908 3.1 -7.21 0.37 + 0.06 $ ^{+0.06}_{-0.37} $ 0.47 0.73 + 0.16 $ ^{+0.16}_{-0.73} $ -ADF, +Δd HII region/indirect [28]
C12b 2 -9.5 0.12 + 0.1 $ ^{+0.1}_{-0.12} $ 1.6 0.067 + 0.032 $ ^{+0.032}_{-0.067} $ -ADF, +Δd HII region/indirect [28]
Ste14a 2.2 -7.38 0.12 + 0.13 $ ^{+0.13}_{-0.12} $ 1.3 0.44 + 0.29 $ ^{+0.29}_{-0.44} $ -ADF, +Δd HII region/indirect [28]
C12c 3.5 -8.61 0.6 + 0.17 $ ^{+0.17}_{-0.6} $ 0.38 2 + 0.14 $ ^{+0.14}_{-2} $ -ADF, +Δd HII region/indirect [28]
KBSS-LM1_stack 2.4 -8.35 0.3 + 0.3 $ ^{+0.3}_{-0.3} $ 1.6 0.21 + 0.13 $ ^{+0.13}_{-0.21} $ -ADF, +Δd HII region/indirect [28]
GOODS-S_41547 2.5 -7.42 0.14 + 0.16 $ ^{+0.16}_{-0.14} $ -0.6 -ADF, +Δd HII region/indirect [28] lower limit
Ste14b 2.3 -7.45 0.12 + 0.08 $ ^{+0.08}_{-0.12} $ 0.07 -ADF, +Δd HII region/indirect [28] lower limit
S13 1.4 -7.52 0.18 + 0.09 $ ^{+0.09}_{-0.18} $ -1.6 -ADF, +Δd HII region/indirect [28] lower limit
B14 3.6 -8.07 0.4 + 0.38 $ ^{+0.38}_{-0.4} $ 1.8 -ADF, +Δd HII region/indirect [28] lower limit
COSMOS_23895 3.6 -7.93 0.08 + 0.14 $ ^{+0.14}_{-0.08} $ 0.96 -ADF, +Δd HII region/indirect [28] lower limit
MOSDEF_composite 2.8 -7.75 0.09 + 0.11 $ ^{+0.11}_{-0.09} $ 0.29 -ADF, +Δd HII region/indirect [28] lower limit
WLM 0 -9.77 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.14 0.11 + 0.11 $ ^{+0.11}_{-0.11} $ +ADF, +Δd BSG [29, 29, 30]
IC1613 0 -10.6 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.26 0.11 + 0.11 $ ^{+0.11}_{-0.11} $ +ADF, +Δd BSG [29, 29, 30]
NGC6822 0 -9.9 0.17 + 0.17 $ ^{+0.17}_{-0.17} $ -0.08 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ +ADF, +Δd BSG [29, 29, 13] ADF = 0.23
NGC55 0 -10.3 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.25 0.12 + 0.12 $ ^{+0.12}_{-0.12} $ +ADF, +Δd BSG [29, 29, 30]
NGC300 0 -10.1 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.13 0.063 + 0.063 $ ^{+0.063}_{-0.063} $ +ADF, +Δd BSG [29, 29, 30] ADF = 0.22
M33 0 -9.92 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.27 0.071 + 0.071 $ ^{+0.071}_{-0.071} $ +ADF, +Δd BSG [29, 29, 30] ADF = 0.27
M31 0 -11.1 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.37 0.23 + 0.23 $ ^{+0.23}_{-0.23} $ +ADF, +Δd BSG [29, 29, 30] ADF = 0.18
M81 0 -10.9 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.23 0.15 + 0.15 $ ^{+0.15}_{-0.15} $ +ADF, +Δd BSG [29, 29, 30]
M83 0 -9.79 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.19 0.28 + 0.28 $ ^{+0.28}_{-0.28} $ +ADF, +Δd BSG [29, 29, 30]
NGC2403 0 -9.92 0.22 + 0.22 $ ^{+0.22}_{-0.22} $ -0.17 0.071 + 0.071 $ ^{+0.071}_{-0.071} $ +ADF, +Δd BSG [31, 31, 30]
- 2.2 -8.75 0.33 0.12 + 0.12 $ ^{+0.12}_{-0.12} $ +ADF, +Δd, -ΔSPS UV cont., BPASS [32] stack, ZO assigned from MZR

Notes. Observational sSFR (column 3) and [O/Fe] (column 4) estimates used in this study. The latter assume log10(O/Fe) = 1.33 dex Grevesse & Sauval (1998). Column 5 lists sources of systematic [O/Fe] offsets between the studies. Unless a different value is specified in the last column, we assume: ADF = 0.24 dex (offset between direct method and recombination line ZO/H scales), Δd = 0.1 dex (oxygen dust depletion correction), ΔICF, Fe = 0.2 dex (ZFe ionisation correction factor), ΔSPS = 0.1 dex (ZFe offset between BPASS and S99 SPS models). The first reference in column 7 points to ZFe, the second to ZO/H, the third to sSFR or SFR and the last (if applicable) to to M*. If only one reference is given, all properties come from the same source.

References. [1] Spina et al. (2022), [2] Arellano-Córdova et al. (2020), [3] Elia et al. (2022), [4] Bland-Hawthorn & Gerhard (2016), [5] Song et al. (2021), [6] Domínguez-Guzmán et al. (2022), [7] Skibba et al. (2012), [8] Lebouteiller et al. (2013), [9] Zhou et al. (2021), [10] Kaufer et al. (2004), [11] Magrini et al. (2005), [12] Hunter et al. (2010), [13] Woo et al. (2008), [14] Hosek (2014), [15] Peña et al. (2007), [16] Cullen et al. (2021), [17] Steidel et al. (2016), [18] Topping et al. (2020), [19] Kojima et al. (2021), [20] Izotov et al. (2018), [21] Thuan et al. (2022), [22] Senchyna et al. (2022), [23] Berg et al. (2016), [24] Senchyna et al. (2019), [25] Senchyna et al. (2017), [26] Strom et al. (2018), [27] Strom et al. (2022), [28] Sanders et al. (2020), [29] Bresolin et al. (2016), [30] Leroy et al. (2019), [31] Bresolin et al. (2022), [32] Kashino et al. (2022)

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