Table 1.
Basic data for the program stars and for the objects taken from the literature.
| Name | Source_id | DR | RA | Dec | Mode | Period | V | ϖ/σϖ | D | E(B − V) |
|---|---|---|---|---|---|---|---|---|---|---|
| deg | deg | days | mag | kpc | mag | |||||
| DR2 6498717390695909376 | 6498717390695909376 | DR2 | 351.00495 | −57.04665 | F | 0.806120 | 13.914 | 8.6 | 7.1 ± 0.6 | 0.014 |
| DR2 2976160827140900096 | 2976160827140900096 | DR3 | 73.77906 | −19.18685 | F | 1.001443 | 15.593 | 1.2 | 15.3 ± 1.3 | 0.043 |
| HE 2324−1255 | 2409340558427973248 | DR3 | 351.82896 | −12.64747 | 1O | 1.107658 | 13.849 | 3.8 | 10.1 ± 0.8 | 0.034 |
| V716 Oph(a) | 4352629469629411840 | DR3 | 247.70599 | −5.50547 | F | 1.115890 | 12.033 | 17.8 | 2.3 ± 0.2 | 0.438 |
| HE 0114−5929 | 4909045712639882496 | DR3 | 19.20812 | −59.23468 | F | 1.116570 | 14.321 | 4.9 | 9.7 ± 0.8 | 0.025 |
| DF Hyi | 4698416118397803776 | DR3 | 25.20499 | −67.49499 | F | 1.122586 | 14.188 | 1.6 | 10.3 ± 0.9 | 0.026 |
| SHM2017 J000.07389−10.22146 | 2422853521974230400 | DR3 | 0.07391 | −10.22146 | F | 1.146828 | 15.073 | 0.6 | 16.4 ± 1.4 | 0.036 |
| BF Ser(a) | 1208200864738741376 | DR3 | 229.11868 | 16.44430 | F | 1.165421 | 11.986 | 9.6 | 3.9 ± 0.3 | 0.033 |
| EK Del(b) | 1400474455952839168 | DR3 | 240.93063 | 50.22592 | F | 1.409596 | 14.081 | 3.3 | 10.4 ± 0.9 | 0.024 |
| OGLE GAL-ACEP-006 | 4627678075752483584 | DR3 | 65.96439 | −76.91187 | F | 1.883580 | 13.015 | 7.5 | 6.2 ± 0.5 | 0.094 |
| CRTS J003041.3−441620 | 4980356188527065472 | DR3 | 7.67244 | −44.27295 | F | 1.900711 | 13.363 | 2.7 | 9.4 ± 0.8 | 0.010 |
| DR2 2648605764784426624 | 2648605764784426624 | DR2 | 343.43880 | −2.81562 | F | 2.253570 | 14.077 | 3.8 | 11.7 ± 1.0 | 0.074 |
Notes. Name is the star identifications on SIMBAD; source_id is the Gaia identifier; DR is the Gaia Data Release; RA and Dec are the equatorial coordinates (J2000); Mode is the pulsation mode; Period is the period of pulsation; V is the visual magnitude; ϖ/σϖ is the relative error on the Gaia parallaxes; D is the distance calculated as described in Appendix C; and E(B − V) is the reddening calculated from the Schlafly & Finkbeiner (2011) maps using the dustmaps package (Green 2018); (a)Kovtyukh et al. (2018); (b)Luck & Lambert (2011).
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