Table B.1
Stellar mass estimates (selected entries only).
| Identifier | Period (d) | M1 (M⊙) | M2 (M⊙) | M3 (M⊙) | M4 (M⊙) | M5 (M⊙) | Madopted (M⊙) |
|---|---|---|---|---|---|---|---|
| LMC3004 | 1.52 | 2.50 ± 0.01 | 2.81 ± 0.01 | 2.94 ± 0.02 | 2.84 ± 0.08 | 2.17 ± 0.01 | 2.81 ± 0.13 |
| LMC1523 | 1.57 | 2.64 ± 0.01 | 2.81 ± 0.01 | 3.03 ± 0.02 | 2.91 ± 0.09 | 2.45 ± 0.01 | 2.81 ± 0.17 |
| LMC3724 | 2.64 | 3.41 ± 0.01 | 3.91 ± 0.01 | 3.96 ± 0.03 | 3.63 ± 0.14 | 3.21 ± 0.01 | 3.63 ± 0.34 |
| LMC3750 | 2.95 | 3.37 ± 0.01 | 3.81 ± 0.01 | 3.86 ± 0.04 | 3.55 ± 0.13 | 3.32 ± 0.01 | 3.55 ± 0.30 |
| LMC2138 | 3.01 | 3.48 ± 0.01 | 3.82 ± 0.01 | 3.94 ± 0.03 | 3.61 ± 0.13 | 3.25 ± 0.01 | 3.61 ± 0.29 |
| LMC3744 | 3.05 | 3.86 ± 0.01 | 4.41 ± 0.01 | 4.46 ± 0.01 | 4.01 ± 0.17 | 2.08 ± 0.01 | 4.01 ± 0.47 |
| LMC4646 | 3.10 | 3.82 ± 0.01 | 4.47 ± 0.01 | 4.45 ± 0.04 | 4.00 ± 0.17 | 3.68 ± 0.01 | 4.00 ± 0.41 |
| LMC3723 | 3.14 | 3.58 ± 0.01 | 4.16 ± 0.01 | 4.15 ± 0.04 | 3.77 ± 0.15 | 3.33 ± 0.01 | 3.77 ± 0.44 |
| LMC3756 | 3.21 | 3.47 ± 0.01 | 3.78 ± 0.01 | 3.90 ± 0.04 | 3.57 ± 0.13 | 3.46 ± 0.01 | 3.57 ± 0.23 |
| LMC3752 | 3.44 | 3.59 ± 0.01 | 3.79 ± 0.01 | 3.96 ± 0.04 | 3.62 ± 0.14 | 3.63 ± 0.01 | 3.63 ± 0.07 |
| LMC3726 | 3.52 | 3.59 ± 0.01 | 4.11 ± 0.01 | 4.10 ± 0.04 | 3.73 ± 0.14 | 3.50 ± 0.01 | 3.73 ± 0.31 |
| LMC0961 | 3.71 | 4.01 ± 0.01 | 4.49 ± 0.01 | 4.55 ± 0.03 | 4.06 ± 0.17 | 3.26 ± 0.01 | 4.06 ± 0.50 |
| LMC1124 | 4.46 | 3.88 ± 0.01 | 4.35 ± 0.01 | 4.34 ± 0.05 | 3.90 ± 0.16 | 3.89 ± 0.01 | 3.90 ± 0.23 |
| LMC3320 | 4.79 | 4.35 ± 0.01 | 4.75 ± 0.01 | 4.81 ± 0.06 | 4.25 ± 0.19 | 4.27 ± 0.01 | 4.35 ± 0.10 |
| SMC3588 | 5.32 | 4.85 ± 0.02 | 5.29 ± 0.01 | 5.35 ± 0.07 | 4.64 ± 0.22 | 4.57 ± 0.02 | 4.85 ± 0.27 |
| SMC2254 | 5.65 | 6.00 ± 0.02 | 6.64 ± 0.02 | 6.69 ± 0.10 | 5.61 ± 0.33 | 5.58 ± 0.03 | 6.00 ± 0.42 |
| LMC1939 | 6.06 | 4.53 ± 0.02 | 4.98 ± 0.01 | 4.97 ± 0.06 | 4.36 ± 0.20 | 4.31 ± 0.02 | 4.53 ± 0.22 |
| LMC1466 | 6.15 | 4.27 ± 0.01 | 4.80 ± 0.01 | 4.72 ± 0.06 | 4.17 ± 0.18 | 4.21 ± 0.02 | 4.27 ± 0.11 |
| LMC0594 | 6.73 | 4.62 ± 0.02 | 5.02 ± 0.01 | 5.01 ± 0.08 | 4.38 ± 0.20 | 4.90 ± 0.02 | 4.90 ± 0.17 |
| LMC1526 | 6.73 | 4.47 ± 0.02 | 4.71 ± 0.01 | 4.77 ± 0.07 | 4.21 ± 0.18 | 4.67 ± 0.01 | 4.67 ± 0.15 |
| LMC1424 | 6.78 | 4.13 ± 0.01 | 4.86 ± 0.01 | 4.62 ± 0.05 | 4.09 ± 0.17 | 3.93 ± 0.02 | 4.13 ± 0.19 |
| LMC1941 | 6.81 | 5.04 ± 0.02 | 6.25 ± 0.01 | 5.82 ± 0.07 | 4.97 ± 0.26 | 4.67 ± 0.03 | 5.04 ± 0.37 |
| LMC1313 | 6.83 | 4.39 ± 0.02 | 4.60 ± 0.01 | 4.67 ± 0.07 | 4.13 ± 0.18 | 4.50 ± 0.01 | 4.50 ± 0.15 |
| LMC1128 | 6.86 | 4.53 ± 0.02 | 4.76 ± 0.01 | 4.83 ± 0.07 | 4.25 ± 0.19 | 4.60 ± 0.01 | 4.60 ± 0.19 |
| LMC1374 | 6.89 | 4.17 ± 0.01 | 4.61 ± 0.01 | 4.53 ± 0.06 | 4.02 ± 0.17 | 4.27 ± 0.01 | 4.27 ± 0.26 |
| LMC1327 | 6.92 | 4.37 ± 0.01 | 4.70 ± 0.01 | 4.70 ± 0.07 | 4.15 ± 0.18 | 4.55 ± 0.01 | 4.55 ± 0.18 |
| … | |||||||
| LMC1113 | 37.56 | 8.57 ± 0.04 | 8.83 ± 0.02 | 8.39 ± 0.33 | 6.63 ± 0.45 | 10.14 ± 0.05 | 8.57 ± 0.27 |
| LMC3158 | 39.19 | 3.83 ± 0.01 | 3.62 ± 0.01 | 3.48 ± 0.08 | 3.15 ± 0.10 | 4.88 ± 0.01 | 3.62 ± 0.20 |
| SMC2706 | 39.20 | 7.81 ± 0.04 | 8.76 ± 0.02 | 7.90 ± 0.24 | 6.30 ± 0.41 | 8.64 ± 0.05 | 7.90 ± 0.75 |
| LMC0512 | 39.40 | 8.40 ± 0.04 | 8.88 ± 0.02 | 8.29 ± 0.33 | 6.56 ± 0.44 | 10.17 ± 0.05 | 8.40 ± 0.48 |
| SMC1797 | 41.21 | 7.70 ± 0.04 | 8.87 ± 0.02 | 7.85 ± 0.22 | 6.26 ± 0.41 | 8.31 ± 0.05 | 7.85 ± 0.46 |
| SMC4444 | 41.83 | 9.90 ± 0.06 | 10.22 ± 0.03 | 9.69 ± 0.43 | 7.49 ± 0.58 | 11.60 ± 0.07 | 9.90 ± 0.33 |
| LMC0943 | 42.24 | 9.64 ± 0.06 | 10.24 ± 0.03 | 9.54 ± 0.41 | 7.39 ± 0.56 | 11.24 ± 0.07 | 9.64 ± 0.60 |
| SMC2470 | 42.75 | 9.09 ± 0.05 | 9.59 ± 0.02 | 8.95 ± 0.34 | 6.99 ± 0.51 | 10.27 ± 0.06 | 9.09 ± 0.50 |
| LMC0461 | 45.17 | 7.77 ± 0.04 | 8.86 ± 0.02 | 7.85 ± 0.24 | 6.25 ± 0.40 | 8.55 ± 0.05 | 7.85 ± 0.70 |
| LMC0966 | 47.38 | 9.33 ± 0.05 | 10.06 ± 0.03 | 9.22 ± 0.33 | 7.17 ± 0.53 | 10.13 ± 0.07 | 9.33 ± 0.74 |
| LMC4663 | 47.96 | 10.96 ± 0.07 | 11.24 ± 0.03 | 10.65 ± 0.50 | 8.10 ± 0.68 | 12.51 ± 0.08 | 10.96 ± 0.33 |
| LMC1290 | 48.38 | 10.00 ± 0.06 | 10.48 ± 0.03 | 9.77 ± 0.70 | 7.53 ± 0.58 | 14.69 ± 0.07 | 10.00 ± 0.49 |
| LMC2253 | 52.37 | 9.24 ± 0.05 | 9.85 ± 0.03 | 9.03 ± 0.36 | 7.03 ± 0.51 | 10.62 ± 0.06 | 9.24 ± 0.61 |
| LMC0992 | 52.87 | 10.61 ± 0.07 | 10.39 ± 0.03 | 10.02 ± 0.47 | 7.68 ± 0.61 | 12.04 ± 0.07 | 10.39 ± 0.38 |
| SMC0921 | 65.94 | 10.12 ± 0.06 | 9.91 ± 0.03 | 9.42 ± 0.62 | 7.27 ± 0.55 | 13.83 ± 0.06 | 9.91 ± 0.50 |
| SMC2099 | 73.62 | 13.14 ± 0.10 | 13.46 ± 0.05 | 12.53 ± 0.66 | 9.24 ± 0.88 | 14.30 ± 0.12 | 13.14 ± 0.63 |
| LMC4691 | 73.90 | 12.24 ± 0.09 | 12.45 ± 0.04 | 11.60 ± 0.61 | 8.66 ± 0.77 | 13.72 ± 0.10 | 12.24 ± 0.66 |
| LMC4689 | 78.51 | 10.54 ± 0.07 | 12.02 ± 0.03 | 10.42 ± 0.46 | 7.90 ± 0.64 | 11.92 ± 0.10 | 10.54 ± 1.39 |
| SMC1502 | 84.30 | 12.27 ± 0.09 | 11.90 ± 0.04 | 11.29 ± 0.76 | 8.45 ± 0.74 | 15.35 ± 0.09 | 11.90 ± 0.62 |
| LMC4628 | 99.20 | 13.56 ± 0.11 | 14.88 ± 0.05 | 13.12 ± 0.83 | 9.57 ± 0.95 | 16.03 ± 0.15 | 13.56 ± 1.33 |
| LMC4629 | 108.70 | 6.77 ± 0.03 | 6.86 ± 0.01 | 6.12 ± 0.33 | 5.01 ± 0.26 | 10.05 ± 0.03 | (6.77 ± 0.66) |
| LMC1591 | 118.62 | 9.50 ± 0.05 | 9.84 ± 0.02 | 8.74 ± 0.39 | 6.77 ± 0.47 | 11.02 ± 0.06 | (9.50 ± 0.76) |
| SMC0417 | 128.20 | 6.71 ± 0.03 | 6.02 ± 0.01 | 5.68 ± 0.62 | 4.69 ± 0.23 | 13.83 ± 0.02 | (6.02 ± 0.70) |
| LMC0619 | 133.78 | 8.74 ± 0.05 | 9.18 ± 0.02 | 8.00 ± 0.21 | 6.28 ± 0.41 | 8.03 ± 0.06 | (8.03 ± 0.77) |
| SMC3611 | 208.80 | 9.60 ± 0.05 | 10.39 ± 0.02 | 8.71 ± 0.33 | 6.71 ± 0.46 | 10.14 ± 0.07 | (9.60 ± 0.79) |
Notes. Column 1: Identifier (sources are sorted by period). Column 2: Period. Column 3: Mass estimate from the period-luminosity-mass-effective temperature-metallicity relation derived in Groenewegen & Jurkovic (2017) based on the models in Bono et al. (2000b). Column 4: Mass estimate from Eq. 1, based on the models of Anderson et al. (2016). Column 5: Mass estimate from the relation in Ragosta et al. (2019). Column 6: Mass estimate from the relation in Pilecki et al. (2018). Column 7: Mass estimate from the relation in Marconi et al. (2020). Column 8: Adopted mass based on the median and the MAD (see text). Values between parenthesis are deemed unreliable and have not been used in the analysis of the mass-luminosity relation and in the calculation of the evolutionary log ɡ and FWG values. The full table is available at the CDS.
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