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Table A.3
Radial velocities with barycentric correction applied. The gravitational redshifts have not been corrected. The typical uncertainty isof the order of 2 km s−1, depending on S/N. There may be a small systematic trend in the radial velocities derived from HRS spectra that were taken in 2019.
| MJD | vrad,B / km s−1 | vrad,A / km s−1 | Spectrograph |
|---|---|---|---|
| 55846.1 | 4.0 | −14.6 | UVES |
| 55846.1 | 4.1 | −15.7 | UVES |
| 55849.1 | 6.0 | −12.2 | UVES |
| 55849.1 | 4.0 | −13.0 | UVES |
| 55908.0 | −1.2 | −5.0 | UVES |
| 57891.0 | −11.7 | 13.5 | HRS |
| 57891.0 | −11.5 | 11.6 | HRS |
| 58437.0 | −3.3 | −3.2 | HRS |
| 58437.0 | −4.2 | −0.3 | HRS |
| 58612.0 | 2.4 | −10.5 | HRS |
| 58612.0 | 2.6 | −9.4 | HRS |
| 58616.0 | 1.9 | −10.7 | HRS |
| 58616.0 | 2.1 | −11.0 | HRS |
| 58617.0 | 2.0 | −8.3 | HRS |
| 58617.0 | 2.3 | −8.8 | HRS |
| 58619.0 | 4.1 | −10.0 | HRS |
| 58619.0 | 2.9 | −7.5 | HRS |
| 58620.0 | 2.5 | −7.6 | HRS |
| 58620.0 | 4.9 | −8.0 | HRS |
| 58621.0 | 3.9 | −8.4 | HRS |
| 58621.0 | 3.8 | −9.0 | HRS |
| 58624.0 | 3.4 | −8.4 | HRS |
| 58624.0 | 3.0 | −7.4 | HRS |
| 58625.0 | 3.4 | −7.4 | HRS |
| 58625.0 | 4.1 | −7.3 | HRS |
| 58626.0 | 3.3 | −7.9 | HRS |
| 58626.0 | 4.1 | −7.2 | HRS |
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