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Table A.1

AGB/RGB ratios and t90 values for the observational sample of calibrating galaxies.

Galaxy AGB/RGB t90/Gyr References
Fornax 0.1570.020+0.021Mathematical equation: $\[0.157_{-0.020}^{+0.021}\]$ 2.40.3+0.9Mathematical equation: $\[2.4_{-0.3}^{+0.9}\]$ 1, 2
NGC 147 0.0960.011+0.011Mathematical equation: $\[0.096_{-0.011}^{+0.011}\]$ 5.70.4+0.9Mathematical equation: $\[5.7_{-0.4}^{+0.9}\]$ 8
NGC 185 0.0700.012+0.012Mathematical equation: $\[0.070_{-0.012}^{+0.012}\]$ 9.31.6+3.Mathematical equation: $\[9.3_{-1.6}^{+3.-}\]$ 8
Cassiopeia III 0.0820.048+0.048Mathematical equation: $\[0.082_{-0.048}^{+0.048}\]$ 4.11.5+2.5Mathematical equation: $\[4.1_{-1.5}^{+2.5}\]$ 9
Andromeda II 0.0970.036+0.049Mathematical equation: $\[0.097_{-0.036}^{+0.049}\]$ 7.60.5+1.5Mathematical equation: $\[7.6_{-0.5}^{+1.5}\]$ 4, 9
Andromeda I 0.0710.030+0.037Mathematical equation: $\[0.071_{-0.030}^{+0.037}\]$ 9.00.9+1.0Mathematical equation: $\[9.0_{-0.9}^{+1.0}\]$ 4, 9
Andromeda VI 0.0750.020+0.020Mathematical equation: $\[0.075_{-0.020}^{+0.020}\]$ 6.40.3+2.7Mathematical equation: $\[6.4_{-0.3}^{+2.7}\]$ 9
Andromeda VII 0.0730.020+0.020Mathematical equation: $\[0.073_{-0.020}^{+0.020}\]$ 7.70.6+2.5Mathematical equation: $\[7.7_{-0.6}^{+2.5}\]$ 9
Lacerta I 0.0420.028+0.028Mathematical equation: $\[0.042_{-0.028}^{+0.028}\]$ 8.61.5+1.0Mathematical equation: $\[8.6_{-1.5}^{+1.0}\]$ 9
Andromeda III < 0.053 10.11.2+1.1Mathematical equation: $\[10.1_{-1.2}^{+1.1}\]$ 4, 9
Sculptor 0.0370.037+0.089Mathematical equation: $\[0.037_{-0.037}^{+0.089}\]$ 10.72.8+1.3Mathematical equation: $\[10.7_{-2.8}^{+1.3}\]$ 5, 2
Antlia 0.2070.044+0.056Mathematical equation: $\[0.207_{-0.044}^{+0.056}\]$ 2.32 6, 7
FM1/F6D1 0.0900.015+0.018Mathematical equation: $\[0.090_{-0.015}^{+0.018}\]$ 5.35 6, 7
Sc22/Sc-dE1 0.1410.022+0.025Mathematical equation: $\[0.141_{-0.022}^{+0.025}\]$ 3.42 6, 7
IKN 0.0820.008+0.009Mathematical equation: $\[0.082_{-0.008}^{+0.009}\]$ 6.17 6, 7
ESO 294-010 0.1030.020+0.025Mathematical equation: $\[0.103_{-0.020}^{+0.025}\]$ 3.78 6, 7
ESO 540-032 0.0930.013+0.015Mathematical equation: $\[0.093_{-0.013}^{+0.015}\]$ 3.45 6, 7
KDG 2 0.2370.043+0.052Mathematical equation: $\[0.237_{-0.043}^{+0.052}\]$ 0.68 6, 7
KK 77 0.1300.010+0.011Mathematical equation: $\[0.130_{-0.010}^{+0.011}\]$ 3.62 6, 7
ESO 410-005 0.1470.020+0.023Mathematical equation: $\[0.147_{-0.020}^{+0.023}\]$ 1.85 6, 7
HS 117 0.1500.021+0.024Mathematical equation: $\[0.150_{-0.021}^{+0.024}\]$ 0.811 6, 7
KDG 63 0.1390.011+0.012Mathematical equation: $\[0.139_{-0.011}^{+0.012}\]$ 1.59 6, 7
UGC 8833 0.2060.025+0.029Mathematical equation: $\[0.206_{-0.025}^{+0.029}\]$ 1.20 6, 7
KDG 64 0.1470.011+0.012Mathematical equation: $\[0.147_{-0.011}^{+0.012}\]$ 1.41 6, 7
KDG 61 0.1210.009+0.010Mathematical equation: $\[0.121_{-0.009}^{+0.010}\]$ 1.30 6, 7
DDO 181 0.1930.016+0.018Mathematical equation: $\[0.193_{-0.016}^{+0.018}\]$ 1.12 6, 7
KKH 98 0.1670.032+0.040Mathematical equation: $\[0.167_{-0.032}^{+0.040}\]$ 1.23 6, 7
KDG 73 0.1840.035+0.043Mathematical equation: $\[0.184_{-0.035}^{+0.043}\]$ 1.74 6, 7
KKH 37 0.1400.017+0.019Mathematical equation: $\[0.140_{-0.017}^{+0.019}\]$ 1.54 6, 7
UGCA 292 0.1520.038+0.051Mathematical equation: $\[0.152_{-0.038}^{+0.051}\]$ 0.59 6, 7
DDO 113 0.1220.017+0.020Mathematical equation: $\[0.122_{-0.017}^{+0.020}\]$ 1.53 6, 7
DDO 44 0.1470.013+0.014Mathematical equation: $\[0.147_{-0.013}^{+0.014}\]$ 1.45 6, 7
GR8 0.1550.027+0.032Mathematical equation: $\[0.155_{-0.027}^{+0.032}\]$ 1.64 6, 7
DDO 78 0.1210.009+0.010Mathematical equation: $\[0.121_{-0.009}^{+0.010}\]$ 1.37 6, 7
DDO 6 0.1500.019+0.021Mathematical equation: $\[0.150_{-0.019}^{+0.021}\]$ 1.41 6, 7
UGC 8508 0.1760.015+0.016Mathematical equation: $\[0.176_{-0.015}^{+0.016}\]$ 1.11 6, 7
NGC 3741 0.1700.016+0.018Mathematical equation: $\[0.170_{-0.016}^{+0.018}\]$ 1.104 6, 7
KDG 52 0.1530.028+0.034Mathematical equation: $\[0.153_{-0.028}^{+0.034}\]$ 2.04 8, 10
DDO 53 0.2130.016+0.017Mathematical equation: $\[0.213_{-0.016}^{+0.017}\]$ 1.19 6, 7

Notes. References: 1) de Boer et al. (2012), 2) Weisz et al. (2015), 3) Hubble Source Catalog photometry WFC3 F606W/F814W (GO-15336; PI: A. Ferguson), 4) Skillman et al. (2017), 5) de Boer et al. (2011), 6) Dalcanton et al. (2009), 7) Weisz et al. (2011), 8) Geha et al. (2015), 9) Savino et al. (2025)

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