Table I.2
Measurements of the radial velocity of our targets.
| Target | Time (JD) [d] | vR,Tell | vR,BC | vR,⋆ | ![]() |
![]() |
![]() |
![]() |
t–test |
|---|---|---|---|---|---|---|---|---|---|
| HR 8799 e | 2460233.618 | ![]() |
−12.11 | −10.4 ± 0.2 | ![]() |
![]() |
![]() |
![]() |
−164 |
| HR 8799 c | 2460256.526 | ![]() |
−20.63 | −10.4 ± 0.2 | ![]() |
![]() |
![]() |
![]() |
−385 |
| 2MJ0219 b | 2460256.605 | ![]() |
−10.38 | 12.0 ± 1.9 | ![]() |
![]() |
![]() |
![]() |
73 |
| AF Lep b | 2460256.729 | ![]() |
13.96 | 21.1 ± 0.4 | ![]() |
![]() |
![]() |
![]() |
−253 |
| HR 2562 B | 2460256.855 | ![]() |
4.38 | 26.2 ± 0.2 | ![]() |
![]() |
![]() |
![]() |
186 |
| HIP 79098 AB B (n1) | 2460354.825 | ![]() |
29.94 | ![]() |
![]() |
![]() |
![]() |
−3089 | |
| HIP 79098 AB B (n2) | 2460356.863 | ![]() |
30.03 | ![]() |
![]() |
![]() |
![]() |
−664 | |
| ROXs 42 B b | 2460354.886 | ![]() |
29.25 | −0.7 ± 13.4 | ![]() |
![]() |
![]() |
![]() |
−103 |
| AB Pic b | 2460355.553 | ![]() |
−2.84 | 22.0 ± 0.2 | ![]() |
![]() |
![]() |
![]() |
403 |
| CT Cha b | 2460355.688 | ![]() |
12.25 | ![]() |
![]() |
![]() |
![]() |
95 | |
| VHS 1256 b | 2460355.785 | ![]() |
23.99 | ![]() |
![]() |
![]() |
![]() |
−631 | |
| HIP 78530 B | 2460355.831 | ![]() |
30.18 | −4.7 ± 0.9 | ![]() |
![]() |
![]() |
![]() |
169 |
| ROXs 12 b | 2460355.892 | ![]() |
29.44 | −8.0 ± 5.4 | ![]() |
![]() |
![]() |
![]() |
−508 |
Notes. All radial velocities are given in units of kms−1. We use the following notation: vR,Tell is our measured RV of the tellurics; vR,BC is the RV of the observatory towards the target vR,⋆ is the RV of the star as measured by GAIA; vR,P is our measured RV of the planet; ΔvR,P⋆ is our final measurement of the RV of the planet relative to its star (if the stellar RV is not available, then ΔvR,P⋆ indicates the RV of the planet relative to the solar barycentre); finally, the superscript denotes which molecular spectral template (CO or H2O) was used. The final values are obtained using the formula ΔvR,P⋆ = vR,P − vR,Tell − vR,⋆ + vR,BC. The last column indicates the result of a Welch’s t–test between the bootstrap samples obtained from the RV measurement using the spectral templates of CO and H2O. The further a t–test value is from zero (positive or negative), the larger is the inconsistency between the RV measurements performed with the CO and H2O templates.
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