Table 3
HARPS and FIES RV measurements of the CoRoT-33 system.
| Instrument | BJD | vrad [km s-1] | Uncertainty [km s-1] | FWHM | BIS | S/N | |||
|
|
|||||||||
| HARPS | 56 471.70867 | 27.159 | 0.240 | 10.8 | −0.08 | 1.1 (moon) | |||
| HARPS | 56 473.65935 | 14.793 | 0.033 | 10.1 | −0.04 | 7.4 | |||
| HARPS | 56 474.75692 | 16.348 | 0.127 | 9.5 | −0.06 | 2.0 | |||
| HARPS | 56 475.74925 | 23.725 | 0.051 | 9.9 | −0.07 | 5.1 | |||
| HARPS | 56 509.71203 | 16.736 | 0.058 | 10.1 | 0.03 | 4.6 | |||
| HARPS | 56 516.59952 | 24.455 | 0.040 | 9.9 | −0.12 | 6.0 | |||
| HARPS | 56 518.67738 | 25.197 | 0.032 | 9.9 | −0.06 | 7.4 | |||
| HARPS | 56 519.64904 | 18.248 | 0.085 | 10.0 | 0.04 | 3.3 (moon) | |||
| FIES | 56 841.58071 | 17.967 | 0.026 | 12.9 | 0.014 | 20 | |||
| FIES | 56 842.62444 | 25.419 | 0.033 | 12.7 | −0.056 | 18 | |||
| FIES | 56 843.60496 | 28.120 | 0.036 | 12.5 | −0.044 | 16 | |||
| FIES | 56 844.61337 | 24.856 | 0.046 | 12.6 | 0.006 | 15 | |||
Notes. FWHM is the average full-width at half maximum of the lines used (in Ångström) and BIS is the corresponding bisector spans. S/N is the signal-to-noise ratio of the individual spectra. The FWHM of the FIES CCFs are wider than those extracted from the HARPS spectra because of the different resolutions of the two spectrographs.
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