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Table 3

Stellar parameters and metallicities from the UVES and UES spectra.

HD Teff δ Teff log g δlog g ξt δ ξt [Fe/H] δ [Fe/H]

[K] [K] [dex] [dex] [kms-1] [kms-1] [dex] [dex]

209 458a 6118 22 4.50 0.04 1.21 0.03 0.03 0.02
2039a 5959 31 4.45 0.04 1.26 0.03 0.32 0.02
213 240 6022 19 4.27 0.05 1.25 0.02 0.14 0.01
23 596b 6134 35 4.25 0.08 1.30 0.04 0.31 0.03
33 636 5994 17 4.71 0.02 1.79 0.02 –0.08 0.01
50 554b 6129 50 4.41 0.07 1.11 0.06 0.01 0.04
52 265a 6136 46 4.36 0.04 1.32 0.06 0.21 0.03
72 659 5951 13 4.30 0.02 1.42 0.01 0.03 0.01
74 156 6099 19 4.34 0.03 1.38 0.02 0.16 0.01
89 744b 6349 43 3.98 0.05 1.62 0.05 0.22 0.03
9826 b 6292 43 4.26 0.06 1.69 0.05 0.13 0.03

Notes.Stellar parameters, Teff and log (g/cm s2), microturbulent velocities, ξt, and metallicities , [Fe/H], and their uncertainties, of the planet-host stars observed with UVES/VLT and UES/WHT spectrographs.

(a)

Stars observed with the UVES spectrograph at VLT telescope at λ/δλ ~ 110 000. The other stars were observed with UVES at λ/δλ ~ 85 000.

(b)

Stars observed with the UES spectrograph at WHT telescope at λ/δλ ~ 65 000.

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