Table 1
Sample of stars (selected entries).
| Identifier | HV | Period (days) | d (kpc) | AV (mag) | Teff (K) | log ɡ (cgs) | Ref | Luminosity (L⊙) | Teff (K) | R (R⊙) | Mass (M⊙) | log ɡ (cgs) | log ɡF (cgs) |  |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| LMC0046 | 12717 | 8.844 | 50.62 | 0.39 | 5224 ± 134 | 2.45 ± 0.19 | (5) | 3777.1 ± 88.3 | 5750 ± 125 | 62.0 ± 2.7 | 5.50 ± 0.22 | 1.59 ± 0.04 | 2.55 ± 0.05 | 9.5 |
| LMC0079 | -1 | 22.544 | 50.52 | 0.36 | 6150 ± 97 | 1.50 ± 0.10 | (4) | 7823.3 ± 102.0 | 5125 ± 88 | 112.4 ± 3.8 | 6.58 ± 0.44 | 1.16 ± 0.04 | 2.32 ± 0.05 | 6.1 |
| LMC0107 | 12452 | 8.739 | 50.48 | 0.43 | 5390 ± 42 | 0.80 ± 0.07 | (1) | 3834.1 ± 91.3 | 5750 ± 125 | 62.5 ± 2.7 | 5.68 ± 0.25 | 1.60 ± 0.05 | 2.57 ± 0.06 | 6.7 |
| LMC0328 | 873 | 34.449 | 50.75 | 0.24 | 5222 ± 27 | 1.25 ± 0.06 | (5) | 17626.4 ± 335.4 | 5250 ± 144 | 160.8 ± 8.6 | 8.80 ± 0.40 | 0.97 ± 0.05 | 2.09 ± 0.07 | 7.0 |
| LMC0367 | 872 | 29.822 | 49.79 | 0.24 | 5675 ± 120 | (5) | 9577.3 ± 137.1 | 5000 ± 125 | 130.6 ± 6.4 | 6.38 ± 0.56 | 1.01 ± 0.06 | 2.22 ± 0.07 | 16.7 | |
| LMC0434 | 875 | 30.349 | 50.25 | 0.26 | 5660 ± 100 | 0.30 ± 0.13 | (2) | 17254.3 ± 617.9 | 5625 ± 144 | 138.6 ± 7.3 | 7.22 ± 0.36 | 1.02 ± 0.05 | 2.02 ± 0.07 | 5.2 |
| LMC0461 | 877 | 45.166 | 49.86 | 0.26 | 4890 ± 109 | 0.70 ± 0.08 | (1) | 14891.6 ± 257.9 | 4750 ± 125 | 180.5 ± 9.3 | 7.85 ± 0.70 | 0.82 ± 0.06 | 2.12 ± 0.08 | 13.6 |
| LMC0467 | 876 | 22.720 | 49.70 | 0.23 | 5391 ± 74 | 1.63 ± 0.16 | (5) | 9500.7 ± 251.0 | 5375 ± 125 | 112.6 ± 5.3 | 6.54 ± 0.22 | 1.16 ± 0.05 | 2.23 ± 0.06 | 4.4 |
| LMC0501 | 878 | 23.311 | 50.37 | 0.24 | 5130 ± 77 | 0.30 ± 0.05 | (2) | 10708.0 ± 279.0 | 5500 ± 125 | 114.2 ±5.2 | 6.62 ± 0.12 | 1.14 ± 0.04 | 2.18 ± 0.05 | 4.6 |
| LMC0504 | 12505 | 14.393 | 50.05 | 0.33 | 3867.4 ± 132.1 | 5000 ± 189 | 83.0 ± 6.1 | 5.63 ± 0.32 | 1.35 ± 0.07 | 2.55 ± 0.09 | 20.6 | |||
| LMC0510 | 879 | 36.831 | 50.22 | 0.34 | 5530 ± 64 | 0.10 ± 0.15 | (2) | 13853.0 ± 335.2 | 4875 ± 153 | 165.3 ± 10.1 | 8.48 ± 0.53 | 0.93 ± 0.06 | 2.18 ± 0.08 | 33.5 |
| LMC0512 | 2257 | 39.398 | 50.36 | 0.22 | 5200 ± 79 | 0.00 ± 0.09 | (2) | 17977.8 ± 152.2 | 5125 ± 88 | 170.4 ± 5.8 | 8.40 ± 0.48 | 0.90 ± 0.04 | 2.07 ± 0.05 | 6.2 |
| LMC0528 | 881 | 35.731 | 50.47 | 0.15 | 5200 ± 64 | 0.10 ± 0.08 | (2) | 15023.5 ± 494.6 | 5125 ± 189 | 155.7 ± 11.2 | 7.70 ± 0.46 | 0.95 ± 0.07 | 2.11 ± 0.10 | 21.2 |
| LMC0545 | 2262 | 15.832 | 50.38 | 0.25 | 5420 ± 85 | 0.80 ± 0.05 | (2) | 5898.8 ± 124.2 | 5250 ± 125 | 93.0 ± 4.4 | 6.52 ± 0.38 | 1.31 ± 0.05 | 2.43 ± 0.06 | 7.3 |
| LMC0546 | 2249 | 15.216 | 49.64 | 0.21 | 6730 ± 285 | 1.40 ± 0.29 | (5) | 6215.9 ± 160.9 | 5500 ± 189 | 87.0 ±5.8 | 5.99 ± 0.25 | 1.34 ± 0.06 | 2.38 ± 0.08 | 16.2 |
| LMC0561 | 880 | 11.670 | 49.73 | 0.22 | 5383 ± 202 | 2.18 ± 0.26 | (5) | 4836.7 ± 88.8 | 5875 ± 168 | 67.2 ± 3.7 | 4.72 ± 0.15 | 1.45 ± 0.05 | 2.38 ± 0.07 | 7.1 |
| LMC0590 | 882 | 31.787 | 50.18 | 0.31 | 5880 ± 322 | 0.00 ± 0.10 | (2) | 14075.5 ± 307.3 | 5250 ± 153 | 143.7 ± 8.2 | 7.48 ± 0.29 | 1.00 ± 0.06 | 2.12 ± 0.08 | 16.6 |
| LMC0594 | -1 | 6.733 | 50.19 | 0.27 | 5520 ± 194 | 0.90 ± 0.05 | (2) | 2245.8 ± 44.7 | 5625 ± 189 | 50.0 ± 3.2 | 4.90 ± 0.17 | 1.73 ± 0.06 | 2.73 ± 0.08 | 17.2 |
| LMC0619 | 883 | 133.779 | 49.89 | 0.28 | 4754 ± 11 | 1.65 ± 0.02 | (5) | 48057.0 ± 2103.3 | 4625 ± 208 | 342.0 ± 29.8 | (8.03 ± 0.77) | (0.27 ± 0.08) | (1.61 ± 0.11) | 86.4 |
| LMC0648 | 2270 | 13.626 | 50.17 | 0.28 | 5300 ± 90 | 0.50 ± 0.07 | (2) | 4192.2 ± 109.1 | 5250 ± 125 | 78.4 ± 3.7 | 5.53 ± 0.31 | 1.39 ± 0.05 | 2.51 ± 0.06 | 7.4 |
| … | ||||||||||||||
| SMC3533 | 1950 | 7.990 | 62.44 | 0.13 | 5900 ± 100 | 1.64 ± 0.10 | (6) | 3226.2 ± 123.4 | 5375 ± 189 | 65.6 ± 4.6 | 6.86 ± 0.89 | 1.65 ± 0.08 | 2.72 ± 0.10 | 24.8 |
| SMC3565 | 1954 | 16.694 | 62.44 | 0.15 | 5890 ± 100 | 1.00 ± 0.10 | (3) | 9712.3 ± 285.1 | 5500 ± 153 | 108.7 ± 6.0 | 8.97 ± 0.66 | 1.32 ± 0.06 | 2.36 ± 0.08 | 13.8 |
| SMC3588 | 1957 | 5.319 | 62.44 | 0.12 | 5975 ± 100 | 1.84 ± 0.10 | (6) | 1964.1 ± 75.0 | 5750 ± 189 | 44.7 ± 2.9 | 4.85 ± 0.27 | 1.83 ± 0.06 | 2.79 ± 0.08 | 16.0 |
| SMC3611 | 1956 | 208.799 | 62.44 | 0.10 | 5677 ± 63 | 1.94 ± 0.19 | (5) | 69071.1 ± 2229.5 | 4375 ± 168 | 458.2 ± 34.0 | (9.60 ± 0.79) | (0.10 ± 0.07) | (1.54 ± 0.10) | 37.4 |
| SMC4555 | 2209 | 22.642 | 62.44 | 0.17 | 6130 ± 100 | 1.10 ± 0.10 | (3) | 14112.7 ± 430.0 | 5625 ± 153 | 125.3 ±6.8 | 8.64 ± 0.08 | 1.18 ± 0.04 | 2.18 ± 0.06 | 18.0 |
| SMC4697 | 817 | 18.901 | 62.44 | 0.12 | 5850 ± 100 | 1.00 ± 0.10 | (3) | 9953.4 ± 533.2 | 5500 ± 237 | 110.1 ± 9.4 | 7.91 ± 0.35 | 1.26 ± 0.08 | 2.30 ± 0.11 | 59.7 |
| SMC4919 | 6357 | 33.338 | 62.44 | 0.18 | 6130 ± 100 | 0.50 ± 0.10 | (3) | 21581.7 ± 924.8 | 5250 ± 204 | 177.9 ± 13.6 | 11.61 ± 0.24 | 1.00 ± 0.07 | 2.12 ± 0.09 | 13.5 |
| SMC4953 | 11211 | 21.386 | 62.44 | 0.09 | 4830 ± 100 | 0.00 ± 0.10 | (3) | 11665.8 ± 387.5 | 5250 ± 153 | 130.8 ± 7.6 | 10.08 ± 0.59 | 1.21 ± 0.06 | 2.33 ± 0.08 | 15.8 |
| SMC4976 | 2231 | 36.737 | 62.44 | 0.17 | 16641.3 ± 1921.0 | 5125 ± 312 | 163.9 ± 20.5 | 8.38 ± 0.55 | 0.93 ± 0.11 | 2.09 ± 0.15 | 47.9 |
Notes. Column 1. The identifier used in this paper, which is related to the identifier used by OGLE. The first entry, LMC0046, for example, would be known as OGLE-LMC-CEP-0046. Column 2. Harvard variable (HV) identifier, when available. Column 3. Pulsation period. Column 4. The adopted distance. For the LMC objects this includes the geometric correction, see Sect. 3.2. Column 5. The adopted reddening value Av based on Skowron et al. (2021), see main text. Column 6. Effective temperature in the literature. For references 3 and 6 an uncertainty of 100 K has been adopted. Column 7. log gravity in the literature. For references 3, 4 and 6 an uncertainty of 0.1 dex has been adopted. Column 8. References for the data in Cols. 6 and 7, (1) Romaniello et al. (2022), re-analysed data from Romaniello et al. (2008; Tables 4 and 6), (2) Romaniello et al. (2022; new spectra, Tables 3 and 5), (3) Romaniello et al. (2008), (4) Lemasle et al. (2017), (5) Sprague et al. (2022). (6) Ragosta et al. (2019; LMC) and Marconi et al. (2017; SMC). For reference (6) the values are not determined from high-resolution spectroscopy but from their best-fitting LC fitting models. Column 9. Luminosity with error bar from the SED fitting. Column 10. (photometric) effective temperature with error bar from the SED fitting. Column 11. Radius with error bar, derived from L and Teff. Column 12. Adopted stellar mass, see Appendix B. Column 13. log gravity determined from mass and radius. Column 14. Flux-weighted gravity calculated from the gravity and Teff. For a few stars the mass estimate is clearly too low given their period and the value for the mass and (flux-weighted) gravity are not used and listed between parenthesis. Column 15. The reduced χ2 of the fit to the SED. The full table is available at the CDS.
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