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Table 2

Solar twins in both samples.

HD number Teff (GCS) Teff (TW) [Fe/H] (GCS) [Fe/H] (TW) log g (TW)
[K] [K] [dex] [dex] [dex]

FE12 sample 78660 5715 5776 0.09 0.06 4.55
97356 5754 5805 0.06 0.02 4.35
117860 5821 5948 0.08 0.13 4.62
126525 5585 5628 0.19 0.02 4.52
138573 5689 5777 0.10 0.00 4.46
142415 5916 5904 0.04 0.08 4.40
146233 5768 5819 0.02 0.08 4.47
147513 5781 5885 0.13 0.04 4.53
163441 5702 5795 0.09 0.09 4.43
173071 5875 6044 0.04 0.25 4.49

FE14 sample 25680 5781 5905 0.08 0.08 4.57
28068 5728 5761 0.04 0.07 4.32
29601 5598 5608 0.14 0.10 4.24
35769 5649 5631 0.12 0.13 4.34
39649 5675 5740 0.09 0.01 4.40
41708 5821 5928 0.07 0.08 4.45
67010 5598 5613 0.20 0.13 4.48
76440 5623 5781 0.23 0.05 4.34
77461 5754 5835 0.18 0.02 4.49

Average ± Scatter 5727 ± 100 5799 ± 128 −0.10 ± 0.07 0.03 ± 0.10 4.45 ± 0.10

Notes. Shown are the GCS-III values and the derived values from this work (TW). We also add our values for log g, as it is also well centred on the solar value of 4.44. Two stars in italics are twins that have only been identified by using other line lists than the Ra09 list adopted in D12, see Sect. 4.2. Stars with a (∗) are considered the best twins in this analysis, see Sect. 6 and Fig. 11c.

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