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Table 2

Spectroscopic parameters with uncertainties for the stars measured in this work.

HIP HD T eff log g ξ t [Fe/H] A(Fe I)⟩ n I A(Fe II)⟩ n II Spec.
(K) (cm s-2) (km s-1) dex
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

Sun 5784 ± 15 4.51 ± 0.03 1.01 ± 0.09 0.02 ± 0.01 7.52 ± 0.02 253 7.52 ± 0.02 26 5

Stars with known debris discs

171 224930 5354 ±15 4.32 ±0.04 0.74 ±0.12 0.83 ±0.01 6.67 ±0.02 208 6.67 ±0.02 18 5
490 105 5967 ±35 4.52 ±0.08 1.76 ±0.26 0.16 ±0.03 7.35 ±0.04 151 7.34 ±0.05 19 7
544 166 5584 ±20 4.73 ±0.05 1.22 ±0.16 0.15 ±0.02 7.65 ±0.03 256 7.65 ±0.03 21 5
1598 1562 5768 ±20 4.56 ±0.04 1.12 ±0.13 0.27 ±0.02 7.23 ±0.02 205 7.23 ±0.03 17 1
1599 1581 5877 ±20 4.25 ±0.04 1.13 ±0.14 0.24 ±0.02 7.26 ±0.02 221 7.26 ±0.03 23 6

Notes. Columns 7 and 9 give the mean iron abundance derived from Fe I and Fe II lines, respectively, while Cols. 8 and 10 give the corresponding number of lines. The rest of the columns are self-explanatory. Only the first five lines are shown here; the full version of the table is available in the electronic edition.

(†)

Spectrograph: (1) CAHA/FOCES; (2) TNG/SARG; (3) NOT/FIES; (4) Mercator/HERMES; (5) S4N-McD; (6) S4N-FEROS; (7) ESO/FEROS; (8) ESO/HARPS.

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