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Table 4

Measurements of spectroscopic parameters from HARPS spectra.

ID1 N JD start JD end RV rms RV vsini FWHM log RHK EW(Li) T eff Remarks
–2 450 000 –2 450 000 (km s-1) (km s-1) (km s-1) (km s-1) (mÅ) (K)

HIP 6177 1 3263. 42.00 7.19 0 5045 ± 17 Zurlo et al. (2013)
HIP 11360 8 4439.68 4479.58 0.81 2.13 ~20 95 pipeline
0.12 SAFIR
HIP 14684 12 3311.79 3805.53 14.72 0.05 10.304 179 5451 ± 7
HIP 32235 17 2948.87 3805.62 20.72 0.13 17.38 18.124 –4.169 239 5493 ± 11
HIP 36948 12 5343.45 5347.47 22.64 0.04 12.830 173 5493 ± 15
TWA 21 24 3402.83 4877.76 18.05 0.17 13.805 –4.06 364 4929 ± 4
TYC 9245-0617-1 1 4594.78 11.49 438 5052 ± 111
HIP 71908 15 7.07 0.15 19.459 subset of data
HIP 72399 1 3409.89 –11.71 14.15 –4.148 0 4903 ± 32
HIP 76829 8 4542.72 4546.72 –7.08 0.63 ~23 0 pipeline
0.03 SAFIR
HIP 79958 1 3828.80 1.74 29.978 117 4838 ± 44
HIP 98470 33 3622.54 5726.84 –10.27 2.02 90 pipeline
0.09 100 SAFIR, subset of data, Lagrange et al. (2009)
HIP 114046 77 2985.57 4392.68 9.00 0.01 3.184 0

Notes. The mean measurement of individual spectra is listed when more than one spectrum is available. For early-type stars we list both the absolute RV obtained with the HARPS pipeline and the RV dispersion of the differential RV obtained with the SAFIR code.

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