Table 1
Stellar parameters for the new C-19 member stars.
| Gaia ID | RA (°) | Dec (°) | G | Telescope/Instrument | texp (s) | S / N1(a) | S / N2(b) | vr (km s−1) | δ(vr) (km s−1) |
|---|---|---|---|---|---|---|---|---|---|
| 28208669730645044482 | 353.39287 | 17.75368 | 13.8 | INT/IDS | 600 | 44 | −190.08 | 2.44 | |
| 27583736527179366402 | 354.57313 | 9.03539 | 14.6 | SDSS | N/A | −156.88 | 0.17 | ||
| 22883134996290026242† | 298.74545 | 74.65642 | 14.1 | Subaru/HDS | 600 | 48 | 23 | −134.29 | 0.67 |
| 26063886414465008641 | 347.06778 | −9.21263 | 17.4 | Magellan/MIKE | 1200 | 8 | 39 | −150.44 | 0.98* |
| 26062421315221235201 | 347.04803 | −9.42817 | 17.0 | Magellan/MIKE | 1200 | 14 | 46 | −135.14 | 0.92* |
| 66007847802235069442 | 339.90245 | −32.79367 | 13.5 | Magellan/MIKE | 600 | 27 | 119 | −41.15 | 0.52* |
| 65593282096956125441 | 327.68642 | −49.38001 | 13.7 | Magellan/MIKE | 600 | 37 | 161 | +32.42 | 0.54* |
| 65947962901429973762 | 335.47287 | −38.35307 | 14.5 | Magellan/MIKE | 600 | 34 | 127 | −22.09 | 0.51* |
| 65678599045307959041 | 331.53238 | −44.04167 | 16.5 | Magellan/MIKE | 1800 | 16 | 68 | +7.45 | 0.83* |
| 26412041617441713923 | 353.47032 | −0.97001 | 14.9 | VLT/UVES | 600 | 9 | 72 | −134.49 | 0.70 |
| 28523300824095257603 | 355.83105 | 24.77643 | 15.3 | VLT/UVES | 600 | 5 | 34 | −191.79 | 0.54 |
| 27608073873462836483 | 351.31022 | 7.96339 | 16.4 | VLT/UVES | 600 | 4 | 36 | −178.60 | 0.64 |
| 28710488555562521603 | 354.48420 | 30.22392 | 16.7 | VLT/UVES | 600 | 2 | 19 | −207.64 | 0.61 |
| 26581159218898494723* | 350.14296 | 2.58381 | 17.1 | VLT/UVES | 600 | 3 | 14 | −172.47 | 0.83 |
| 26449506746007205123 | 350.57152 | −0.22855 | 17.1 | VLT/UVES | 600 | 8 | 54 | −150.23 | 0.98 |
| 26407930131147838723 | 352.99372 | −1.34662 | 17.4 | VLT/UVES | 600 | 7 | 44 | −140.23 | 0.70 |
Notes. The number of the upper script of each star denotes the order of identification in Sect. 2. The star with the dagger symbol has spectra from both Subaru/HDS and INT/IDS, and the radial velocity is derived from the Subaru spectra. The star with the asterisk has low-quality spectra (see details in Sect. 2). (a)S/N per 0.05 Å measured at 5863–5865 Å. (b)S/N per 1 Å measured at 8639–8644 Å. For the six stars observed with MIKE, a systematic uncertainty of 2 km s−1 is assumed and δ(vr) presents statistical uncertainties denoted with an asterisk.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.