Table 2
General statistics of the HARPS observations of the planet-host stars presented in this paper.
Nspectr | ⟨S/N⟩ | Nmeas | ΔT | σRV | ⟨εRV⟩ | |
---|---|---|---|---|---|---|
550 nm | 1-h bin | (days) | (m s−1) | (m s−1) | ||
HD 20003 | 184 | 110 | 184 | 4063 | 5.35 | 0.74 |
HD 20781 | 225 | 112 | 216 | 4093 | 3.41 | 0.76 |
HD 20782a | 71 | 181 | 68 | 4111 | 36.86 | 0.56 |
HD 21693 | 210 | 141 | 210 | 4106 | 4.72 | 0.60 |
HD 31527 | 256 | 180 | 245 | 4135 | 3.19 | 0.64 |
HD 45184 | 308 | 221 | 178 | 4160 | 4.72 | 0.41 |
HD 51608 | 218 | 133 | 216 | 4158 | 4.07 | 0.62 |
HD 134060 | 335 | 199 | 155 | 4083 | 3.68 | 0.40 |
HD 136352 | 649 | 231 | 240 | 3993 | 2.74 | 0.33 |
Notes. Columns are: number of individual spectra observed, ⟨S/N⟩ average signal-to-noise ratio at 550 nm of those spectra, number of measurements obtained after binning the data over 1 h, ΔT the time span of the observations, σRV the rms value of the RV set and ⟨ εRV ⟩ the mean RV photon-noise + calibration error. (a)Star already known as a planet host for which we give here an updated orbit including HARPS observations.
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