Table 2.
Radial velocity catalogs.
| Star | RA | Dec | Date | S/N | Teff | [M/H] | vsini | RV | σ |
|---|---|---|---|---|---|---|---|---|---|
| OBSID | (deg) | (deg) | (MJD) | (K) | (dex) | (km s−1) | (km s−1) | (km s−1) | |
| 693504025 | 33.1157 | 58.6092 | 58446.8958 | 157 | 21 579 | −0.25 | 41 | −96.90 | 0.64 |
| 715104025 | 33.1157 | 58.6092 | 58494.8132 | 135 | 21 579 | −0.25 | 41 | −96.42 | 0.39 |
| 685011073 | 35.0524 | 60.0624 | 58421.0583 | 168 | 22 265 | −0.28 | 53 | −56.78 | 0.42 |
| 702711073 | 35.0524 | 60.0624 | 58468.825 | 163 | 22 265 | −0.28 | 53 | −55.20 | 0.42 |
| 702712188 | 36.9131 | 60.2170 | 58468.841 | 115 | 18 023 | −0.46 | 135 | −56.41 | 1.22 |
| 685012188 | 36.9131 | 60.2170 | 58421.0417 | 115 | 18 023 | −0.46 | 135 | −52.87 | 1.25 |
Notes.
This table is available in its entirety in machine-readable form at the CDS. The typical uncertainties of Teff, [M/H], and vsini are 2185 K, 0.2 dex, (here we use the SLAM [model] error at the S/N = 20 [the maximum value of error], as shown in Fig. 4 of Guo et al. 2021. The high-resolution comparison spectra give individual element abundances rather than [M/H]. Guo et al. 2021 therefore did not give a typical uncertainty of [M/H]) and 11 km s−1, respectively.
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