Table 1.
Global and asteroseismic parameters of the targets with confirmed detection.
WID | GaiaeDR3 ID | RA (J2000) | Dec (J2000) | Vdr (mag) | CUBI (mag) | Teff (K) | L/L⊙ | νmax (μHz) | Δν (μHz) | POPSpec | POPCUBI |
---|---|---|---|---|---|---|---|---|---|---|---|
W491 | 6045479078332149632 | 245.798065 | –26.444676 | 13.757 | –2.059 | 4788 | 37.865 ± 4.083 | 38.724 ± 0.965 | 4.616 ± 0.180 | 2G | 2G |
W508 | 6045478047540140544 | 245.800242 | –26.495482 | 14.307 | –2.096 | 4926 | 21.765 ± 2.192 | 75.929 ± 2.367 | 7.613 ± 0.231 | – | 2G |
W760 ( * ) | 6045477841381440384 | 245.820424 | –26.496654 | 13.129 | –2.038 | 4668 | 71.180 ± 7.748 | 18.148 ± 1.024 | 2.558 ± 0.081 | 2G | 2G |
W779 | 6045479490649030272 | 245.822060 | –26.416080 | 14.059 | –2.114 | 4844 | 28.142 ± 3.030 | 53.392 ± 2.258 | 6.056 ± 0.171 | – | 1G |
W799 | 6045478288058130304 | 245.823516 | –26.452857 | 13.313 | –1.915 | 5596 | 45.743 ± 4.332 | 33.108 ± 1.851 | 4.543 ± 0.117 | – | rHB |
W837 | 6045478081899629696 | 245.825992 | –26.485369 | 14.842 | –2.071 | 5030 | 12.892 ± 1.235 | 123.780 ± 3.537 | 11.765 ± 0.309 | – | 2G |
W1068 | 6045478184978847616 | 245.839217 | –26.475993 | 14.307 | –2.076 | 4900 | 21.934 ± 2.229 | 71.632 ± 2.839 | 7.449 ± 0.301 | – | 2G |
W1091 | 6045478666015246592 | 245.840398 | –26.446373 | 13.488 | –2.054 | 4787 | 48.529 ± 5.227 | 31.402 ± 1.722 | 3.899 ± 0.296 | NC | 2G |
W1156 | 6045477910100876544 | 245.843863 | –26.495077 | 14.053 | –2.134 | 4858 | 28.109 ± 3.026 | 50.740 ± 0.995 | 5.375 ± 0.272 | – | 1G |
W1225 | 6045477978820371712 | 245.847568 | –26.486060 | 13.440 | –1.983 | 5326 | 43.459 ± 4.203 | 34.333 ± 1.907 | 5.279 ± 0.364 | – | rHB |
W1582 | 6045477944460600960 | 245.866076 | –26.486544 | 14.293 | –2.138 | 4885 | 22.325 ± 2.271 | 72.196 ± 2.312 | 7.132 ± 0.440 | – | 1G |
W1608 | 6045478734734712832 | 245.867277 | –26.435713 | 13.228 | –1.985 | 5421 | 51.551 ± 4.936 | 30.400 ± 2.277 | 4.385 ± 0.111 | – | rHB |
W1717 | 6045478730423545984 | 245.872427 | –26.441030 | 14.364 | –2.061 | 4966 | 20.374 ± 2.016 | 83.731 ± 1.718 | 8.619 ± 0.680 | – | 2G |
W1763 | 6045503057118542208 | 245.874265 | –26.390373 | 12.973 | –2.042 | 4616 | 84.140 ± 9.199 | 14.920 ± 1.461 | 2.212 ± 0.078 | 2G | 2G |
W1912 | 6045478764783374208 | 245.880406 | –26.421051 | 14.577 | –2.075 | 4994 | 16.636 ± 1.628 | 100.116 ± 2.931 | 10.021 ± 1.264 | – | 2G |
W2021 | 6045466571386686208 | 245.884849 | –26.489523 | 13.918 | –2.140 | 4841 | 32.030 ± 3.448 | 44.785 ± 1.422 | 5.374 ± 0.229 | 1G | 1G |
W2022 ( * ) | 6045478528576252288 | 245.884878 | –26.439056 | 13.024 | –2.115 | 4677 | 77.933 ± 8.468 | 15.986 ± 1.047 | 2.418 ± 0.085 | 1G** | 1G |
W2034 | 6045502305515873024 | 245.885444 | –26.409477 | 13.498 | –2.135 | 4764 | 48.533 ± 5.240 | 26.413 ± 1.714 | 3.480 ± 0.204 | – | 1G |
W2162 | 6045478356777481984 | 245.890859 | –26.463824 | 13.649 | –2.096 | 4782 | 41.995 ± 4.528 | 35.280 ± 1.784 | 4.245 ± 0.359 | 2G | 2G |
W2386 | 6045478558624847488 | 245.899759 | –26.439063 | 13.440 | –2.054 | 5314 | 43.543 ± 4.214 | 36.400 ± 0.726 | 5.207 ± 0.178 | – | rHB |
W2665 ( * ) | 6045501961918453504 | 245.911909 | –26.428551 | 13.084 | –2.036 | 4675 | 73.824 ± 8.007 | 17.806 ± 0.445 | 2.526 ± 0.089 | 2G | 2G |
W2678 | 6045502477314585728 | 245.912264 | –26.369307 | 13.555 | –2.128 | 4805 | 45.290 ± 4.884 | 31.495 ± 0.878 | 3.862 ± 0.300 | 1G | 1G |
W2887 | 6045466433947664256 | 245.922274 | –26.485789 | 13.418 | –1.926 | 5614 | 41.411 ± 3.922 | 39.876 ± 2.520 | 3.938 ± 0.204 | – | rHB |
W3033 ( * ) | 6045466674465880064 | 245.929551 | –26.468741 | 13.582 | –2.058 | 4785 | 44.566 ± 4.798 | 32.892 ± 1.396 | 4.102 ± 0.334 | 2G | 2G |
W3041 | 6045490210887898368 | 245.930070 | –26.444946 | 14.191 | –2.168 | 4927 | 24.184 ± 2.472 | 62.427 ± 2.156 | 6.847 ± 0.872 | – | 1G |
W3073 | 6045501996278180992 | 245.931331 | –26.427090 | 14.217 | –2.082 | 4868 | 24.146 ± 2.600 | 61.963 ± 1.000 | 6.873 ± 0.374 | – | 2G |
W3480 | 6045466399577821440 | 245.954138 | –26.488691 | 13.816 | –2.096 | 4875 | 34.725 ± 3.550 | 45.087 ± 1.775 | 5.228 ± 0.182 | NC | 2G |
W3528 | 6045466399587848704 | 245.957287 | –26.481054 | 14.070 | –2.152 | 4929 | 27.020 ± 2.737 | 59.026 ± 3.100 | 6.341 ± 0.195 | – | 1G |
W3564 | 6045465643673557760 | 245.959422 | –26.490526 | 13.505 | –2.008 | 4803 | 47.534 ± 5.117 | 31.958 ± 2.938 | 4.029 ± 0.230 | 2G | 2G |
W3742 | 6045489901650196864 | 245.970856 | –26.468500 | 13.653 | –2.157 | 4720 | 42.973 ± 4.649 | 35.071 ± 1.680 | 4.126 ± 0.280 | 1G | 1G |
W3929 ( * ) | 6045490103497000320 | 245.985488 | –26.424575 | 13.428 | –1.940 | 5595 | 41.541 ± 3.942 | 38.242 ± 1.957 | 4.811 ± 0.297 | – | rHB |
W4488 | 6045489351894331776 | 246.061253 | –26.454663 | 13.509 | –2.065 | 4708 | 49.304 ± 5.316 | 27.586 ± 1.425 | 4.324 ± 0.146 | – | 2G |
Targets with more uncertain photometry | |||||||||||
W1512 | 6045479593728227072 | 245.863124 | –26.40367 | – | – | – | – | 39.516 ± 1.704 | 5.401 ± 0.154 | – | NO |
W3079 | 6045490210887906176 | 245.931592 | –26.43842 | – | – | – | – | 34.562 ± 1.228 | 3.852 ± 0.173 | – | NO |
W3474 | 6045466399587823744 | 245.953973 | –26.48835 | – | – | – | – | 44.461 ± 2.358 | 5.151 ± 0.292 | – | NO |
W4092 | 6045490485765778560 | 245.998091 | –26.42664 | – | – | – | – | 28.065 ± 2.369 | 3.729 ± 0.157 | – | NO |
W4283 | 6045490447094400384 | 246.024697 | –26.42321 | – | – | – | – | 50.277 ± 1.645 | 5.849 ± 0.232 | – | NO |
Notes. Columns are as follows: Name of the star in Wallace et al. (2019), Star ID in the Gaia eDR3 (Gaia Collaboration 2021), right ascension (RA) and declination (Dec), V magnitude from Stetson et al. (2019) corrected for differential reddening, CUBI index, and effective temperature (Teff, 100 K has been assumed as 1σ value). Luminosity in solar units, νmax and Δν in μHz, and, finally, population ID either from spectroscopy (POPSpec) or using the CUBI index (POPCUBI). At the bottom, we report the asteroseismic parameters of the targets with more uncertain photometry in the Stetson et al. (2019) data. 1G: first generation. 2G: second generation. NC: not certain. rHB: red horizontal branch star. ( * )Also in Miglio et al. (2016), ( * *)diverging identification: 1G in Marino et al. (2008) and 2G in Carretta et al. (2009); we agree with the former.
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