|Spectrograph||Telescope||Spectral range||λ/δλ||Binning||Nstarsa|||S/N|b||δ |S/N|c||ΔS/Nd|
|HARPS||3.6 m-ESO||3800–6900||110 000||0.010||50||877||429||265–2015|
|UVES||8 m-VLT||4800–6800||85 000||0.016||7||722||150||510–940|
|UES||4.2 m-WHT||4150–7950||65 000||0.029||4||643||180||520–850|
Notes.Details of the spectroscopic data used in this work. The UVES and UES stars are all planet hosts. Three of the UVES stars were observed with a slit of 0.3″ providing a resolving power λ/δλ ~ 110 000.
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