Table 2
Radial velocities of the planet host star CoRoT-11 obtained with the SOPHIE, HARPS (EGGS and standard HARPS mode), COUDÉ@TLS, and HIRES spectrographs.
HJD | RV | σRV | Bisector | Texp | S/N per resolution |
(days) | (km s-1) | (km s-1) | (km s-1) | (s) | element at 5500 Å |
|
|||||
SOPHIE – HE Mode | Vr = −0.920 ± 0.160 | ||||
|
|||||
2454643.60252a | –1.164 | 0.218 | 1402 | 42 | |
2454683.42036 | –0.714 | 0.206 | 1607 | 50 | |
|
|||||
HARPS – EGGS Mode | Vr = −1.229 ± 0.041 | ||||
|
|||||
2454731.52836 | –0.932 | 0.067 | –0.531 | 2700 | 88 |
2454742.51115 | –1.364 | 0.104 | –0.149 | 2700 | 54 |
2454745.51100 | –1.370 | 0.087 | –0.476 | 2700 | 66 |
2454746.51455 | –0.986 | 0.071 | –0.583 | 2700 | 81 |
2454747.51953 | –1.509 | 0.115 | –0.892 | 1800 | 48 |
|
|||||
HARPS – Standard Mode | Vr = −1.336 ± 0.044 | ||||
|
|||||
2455023.66206a | –1.663 | 0.149 | –0.286 | 3600 | 34 |
2455024.63997a | –1.405 | 0.111 | –0.705 | 3600 | 48 |
2455045.69605a | –1.013 | 0.114 | –0.747 | 3600 | 52 |
2455064.60739 | –1.166 | 0.083 | –0.408 | 3300 | 64 |
2455067.51277 | –1.085 | 0.092 | –0.204 | 3300 | 59 |
2455068.49041 | –1.547 | 0.130 | 0.472 | 3300 | 42 |
2455069.51299 | –1.384 | 0.110 | –0.497 | 3300 | 48 |
|
|||||
COUDÉ@TLS | Vr = − 0.640 ± 0.130 | ||||
|
|||||
2455035.46055 | –0.951 | 0.174 | 2 × 1800 | 25 | |
2455057.40390 | –0.541 | 0.175 | 2 × 1800 | 25 | |
|
|||||
HIRES | Vr = − 0.207 ± 0.040 | ||||
|
|||||
2455012.80417 | –0.033 | 0.050 | 1200 | 61 | |
2455013.06216 | 0.181 | 0.086 | 1200 | 71 | |
2455013.78975 | –0.165 | 0.089 | 900 | 54 | |
2455013.80073 | –0.083 | 0.090 | 900 | 56 | |
2455013.81181 | –0.170 | 0.135 | 900 | 56 | |
2455013.82275 | 0.173 | 0.111 | 900 | 57 | |
2455013.83360 | –0.012 | 0.142 | 900 | 57 | |
2455013.84473 | 0.099 | 0.073 | 900 | 56 | |
2455013.85572 | 0.037 | 0.119 | 900 | 56 | |
2455013.86677 | 0.274 | 0.108 | 900 | 55 | |
2455013.87785 | 0.240 | 0.078 | 900 | 55 | |
2455013.88881 | 0.017 | 0.100 | 900 | 56 | |
2455013.89978 | 0.089 | 0.080 | 900 | 56 | |
2455013.91097 | –0.263 | 0.086 | 900 | 54 | |
2455014.05389 | –0.386 | 0.119 | 900 | 58 |
Notes. The systemic velocities for each instrument, as derived from the circular Keplerian fit to the data, are reported on the right of the listed spectrographs. The footnote indicates the RV measurements that have been corrected for moonlight contamination.
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.