Table A.2
Results of the fitting without dust
Identifier | d (kpc) | AV (mag) | Teff (K) | Luminosity (L⊙) | ![]() |
SHd (kpc) | SHAv (mag) | dmax (kpc) | ||
M31-PSO009.76 | 761.18 ± (11.0) | 0.17 | 4625 ± 312 | 16668 ± 2581 | 58.4 | |||||
M31-PSO010.11 | 754.41 ± (11.0) | 0.17 | 4000 ± 347 | 16056 ± 1866 | 47.2 | |||||
M31-PSO010.19 | 757.09 ± (11.0) | 0.17 | 4875 ± 221 | 24892 ± 1554 | 19.7 | |||||
M31-LGGS00415 | 764.20 ± (11.0) | 0.17 | 3800 ± 184 | 30045 ± 4577 | 33.5 | |||||
M31-GDR381279 | 752.32 ± (11.0) | 0.17 | 4000 ± 134 | 23101 ± 3654 | 17.7 | |||||
M31-PSO010.63 | 766.98 ± (11.0) | 0.17 | 4375 ± 198 | 29078 ± 5035 | 32.3 | |||||
M31-GDR369249 | 767.51 ± (11.0) | 0.17 | 4125 ± 250 | 24643 ± 2638 | 39.1 | |||||
M31-VRJ004357 | 754.68 ± (11.0) | 0.17 | 3900 ± 180 | 26440 ± 4805 | 23.5 | |||||
M31-PSO011.09 | 752.91 ± (11.0) | 0.17 | 5125 ± 243 | 19667 ± 1995 | 59.2 | |||||
M31-VRJ004434 | 754.86 ± (11.0) | 0.17 | 4625 ± 208 | 29360 ± 1937 | 84.7 | |||||
M31-GDR387319 | 752.36 ± (11.0) | 0.17 | 4625 ± 237 | 24216 ± 1611 | 47.9 | |||||
M31-GDR375422 | 756.56 ± (11.0) | 0.17 | 4875 ± 289 | 24191 ± 1252 | 63.2 | |||||
SMC-CEP-0417 | 62.44 ± (0.94) | 0.08 | 4875 ± 221 | 72352 ± 2823 | 59.8 | |||||
SMC-CEP-0921 | 62.44 ± (0.94) | 0.10 | 5000 ± 177 | 43383 ± 1032 | 40.2 | |||||
SMC-CEP-1502 | 62.44 ± (0.94) | 0.12 | 5375 ± 198 | 65640 ± 2687 | 58.2 | |||||
SMC-CEP-1977 | 62.44 ± (0.94) | 0.13 | 4875 ± 189 | 29258 ± 677 | 46.5 | |||||
SMC-CEP-2099 | 62.44 ± (0.94) | 0.12 | 5125 ± 189 | 48818 ± 1068 | 37.5 | |||||
SMC-CEP-3611 | 62.44 ± (0.94) | 0.10 | 4250 ± 221 | 64918 ± 4074 | 128.8 | |||||
SMC-Dachs3-5 | 62.44 ± (0.94) | 0.23 | 4750 ± 168 | 21979 ± 365 | 30.0 | |||||
M33-013253 | 844.54 ± (11.0) | 0.17 | 4375 ± 253 | 67771 ± 7606 | 95.2 | |||||
M33-013305 | 843.49 ± (11.0) | 0.17 | 4875 ± 177 | 42087 ± 2642 | 31.3 | |||||
M33-013312 | 842.95 ± (11.0) | 0.17 | 4625 ± 627 | 22999 ± 8364 | 193.7 | |||||
M33-013331 | 843.10 ± (11.0) | 0.17 | 4750 ± 189 | 16893 ± 1049 | 45.5 | |||||
M33-013343 | 842.40 ± (11.0) | 0.17 | 4875 ± 289 | 30123 ± 2067 | 100.5 | |||||
M33-V00021 | 840.00 ± (11.0) | 0.17 | 4875 ± 226 | 22999 ± 1364 | 46.2 | |||||
M33-013405 | 841.16 ± (11.0) | 0.17 | 4625 ± 153 | 19762 ± 1690 | 63.0 | |||||
LMC-CEP-4628 | 49.53 ± (0.55) | 0.31 | 4750 ± 168 | 57131 ± 1199 | 24.7 | |||||
LMC-CEP-4629 | 49.14 ± (0.55) | 0.15 | 4750 ± 237 | 32987 ± 1120 | 69.6 | |||||
LMC-CEP-0619 | 49.89 ± (0.55) | 0.28 | 4750 ± 236 | 48544 ± 1538 | 51.3 | |||||
LMC-CEP-0992 | 49.80 ± (0.55) | 0.22 | 5125 ± 144 | 33980 ± 366 | 9.5 | |||||
LMC-CEP-1591 | 49.43 ± (0.55) | 0.30 | 4875 ± 189 | 49882 ± 1085 | 32.9 | |||||
LMC-CEP-2253 | 49.88 ± (0.55) | 0.31 | 4875 ± 189 | 23982 ± 689 | 23.3 | |||||
LMC-Dachs2-24 | 48.53 ± (0.55) | 0.23 | 4625 ± 189 | 28762 ± 726 | 17.8 | |||||
LMC-CEP-4689 | 48.31 ± (0.55) | 0.21 | 4625 ± 188 | 32283 ± 996 | 48.4 | |||||
LMC-CEP-4691 | 48.53 ± (0.55) | 0.33 | 5375 ± 125 | 50872 ± 599 | 8.6 | |||||
Milky Way Cepheids | ||||||||||
ATO093m31 | 15.78 ± (2.58) | 0.10 | 4125 ± 145 | 1740 ± 87 | 31.2 | 1.12 | ||||
ATO142p20 | 9.72 ± (2.43) | 0.08 | 4125 ± 204 | 2747 ± 181 | 55.2 | 7.36 ± 0.15 | 0.51 ± 0.01 | 0.59 | ||
V708 Car | 3.87 ± (0.33) | 1.33 | 3500 ± 134 | 3619 ± 1130 | 255.0 | 3.87 | ||||
II Car | 7.66 ± (1.24) | 1.41 | 3500 ± 134 | 10082 ± 2377 | 199.4 | 5.11 ± 1.75 | 2.57 ± 0.42 | 5.27 | ||
GD-CEP-1859 | 10.62 ± (3.02) | 3.21 | 3400 ± 100 | 19488 ± 5306 | 230.2 | 6.43 | ||||
BLG-T2CEP-0743 | 8.28 ± (0.03) | 4.10 | 3900 ± 194 | 1254 ± 70 | 83.5 | 5.01 | ||||
BLG-T2CEP-0084 | 8.28 ± (0.03) | 4.28 | 3900 ± 212 | 1716 ± 243 | 139.1 | 10.99 ± 0.98 | 6.31 ± 0.06 | 5.01 | ||
BLG-T2CEP-0761 | 8.28 ± (0.03) | 3.74 | 4250 ± 588 | 671 ± 95 | 478.5 | 7.99 ± 1.54 | 4.82 ± 2.12 | 5.02 | ||
BLG-T2CEP-0131 | 8.28 ± (0.03) | 3.85 | 4125 ± 453 | 818 ± 133 | 486.7 | 5.01 | ||||
GDR404357 | 8.28 ± (0.03) | 2.96 | 4250 ± 333 | 1865 ± 142 | 132.5 | 5.02 | ||||
V1496 Aql | 3.54 ± (0.32) | 3.95 | 5375 ± 264 | 32271 ± 1309 | 69.8 | 3.26 ± 0.18 | 4.85 ± 0.35 | 3.54 | ||
GD-CEP-1505 | 4.05 ± (2.21) | 3.59 | 3000 ± 438 | 137 ± 30 | 1940.0 | 4.05 | ||||
ATO290p18 | 7.82 ± (2.64) | 5.44 | 3600 ± 151 | 6562 ± 1315 | 204.9 | 6.28 | ||||
GDR6746185 | 9.16 ± (1.56) | 0.32 | 4000 ± 115 | 3795 ± 218 | 22.5 | 5.70 ± 0.06 | 0.58 ± 0.01 | 1.16 | ||
ATO292p22 | 12.55 ± (2.18) | 3.01 | 3700 ± 150 | 3720 ± 307 | 60.7 | 8.51 ± 0.91 | 5.59 ± 0.50 | 5.97 | ||
GY Sge | 2.89 ± (0.18) | 3.51 | 4500 ± 189 | 20396 ± 1113 | 43.7 | 2.89 | ||||
ET Vul | 13.94 ± (2.52) | 1.93 | 4500 ± 204 | 17489 ± 544 | 53.7 | 5.72 | ||||
CL Vul | 4.28 ± (0.38) | 4.61 | 4375 ± 221 | 38958 ± 1242 | 43.4 | 4.28 | ||||
S Vul | 4.32 ± (0.33) | 2.58 | 4875 ± 189 | 49736 ± 2351 | 36.5 | 3.99 ± 0.44 | 3.79 ± 1.69 | 4.32 | ||
ATO352p17 | 11.87 ± (2.65) | 0.20 | 4000 ± 221 | 686 ± 37 | 46.3 | 0.62 |
Notes. Column 1. The identifier used in this paper. Column 2. The adopted distance. The error in the distance is listed between parenthesis to indicate that this error is not included in the luminosity error estimate. Column 3. The adopted reddening value AV. Column 4. (photometric) effective temperature with error bar from the SED fitting. Column 5. Luminosity with error bar from the SED fitting (for the fixed distance). Column 6. Reduced chi-squared of the fit. Column 7. Distance with error bar from StarHorse (Anders et al. 2022). Column 8. Reddening value AV from StarHorse. Column 9. The maximum distance to which the 3D reddening model is available.
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