Table A.1: Selected stars with particularly high resemblance to the Sun.
Star $\Delta T_{\rm eff}$ $\Delta \log g$ $\Delta v_{\rm t}$ $\Delta ${Fe/H} M $\log age$ Qage $v_{\rm r+m}$ $A_{\rm Li}$ ${q}_{\rm Li}$ $\sigma$
HIP 7585 +0.2 -0.009 +0.04 +0.067 1.02 9.68 A 2.66 1.84 a 0.391
HIP 8486 +30.2 -0.002 +0.09 -0.055 0.97 9.69 C 2.72 2.55 a 0.608
HIP 9349 +19.7 -0.064 +0.03 +0.012 1.00 9.73 A 2.60 2.06 a 0.332
HIP 11728 -50.7 -0.055 +0.01 +0.033 1.01 9.48 B 2.49 (<1.03) x 0.492
HIP 19925 -19.5 +0.041 -0.01 +0.064 0.99 9.47 C 2.70 1.61 a 0.402
HIP 25002 -54.6 -0.029 +0.09 -0.096 0.99 9.56 C 3.53 2.38 a 0.806
HIP 31965 +10.2 -0.111 +0.01 +0.051 1.01 9.87 A 2.49 1.00 b 0.464
HIP 32673 -30.9 +0.138 -0.07 +0.075 1.02 9.50 B 2.28 (<1.04) x 0.755
HIP 35265 +51.8 -0.055 +0.06 -0.009 1.00 9.79 A 2.24 2.01 a 0.559
HIP 38647 -48.3 -0.028 -0.03 +0.012 1.00 9.43 A 2.83 2.13 a 0.518
HIP 43557 +41.2 -0.030 +0.05 -0.061 1.00 9.80 A 3.43 1.50 a 0.579
HIP 49728 -21.1 -0.044 -0.02 -0.064 1.00 9.60 C 2.41 (<1.05) x 0.422
HIP 49756 -35.1 -0.145 +0.01 +0.027 1.02 9.58 C 2.51 1.34 a 0.614
HIP 55459 +51.1 -0.037 +0.03 +0.072 1.03 9.58 A 2.70 1.58 a 0.591
HIP 59610 +59.1 -0.129 +0.07 -0.066 1.02 9.63 B 2.57 1.62 a 0.812
HIP 62816 +31.8 -0.028 -0.08 +0.069 1.02 9.49 B 3.68 2.16 a 0.624
HIP 64150 -14.4 +0.014 +0.03 +0.067 1.04 9.63 B 2.56 (<1.04) x 0.397
HIP 75676 -6.0 -0.031 -0.08 -0.090 0.98 9.62 A 2.54 (<1.07) x 0.614
HIP 76114 -34.0 +0.056 +0.00 -0.003 1.01 9.59 C 2.23 0.91 b 0.388
HIP 79672 +1.7 -0.056 -0.03 +0.039 1.02 9.66 A 2.66 1.63 a 0.309
HIP 88194 -49.2 -0.043 +0.01 -0.071 0.97 9.67 C 2.25 (<0.83) x 0.625
HIP 96901 -24.2 -0.121 +0.00 +0.086 1.01 9.77 B 2.38 (<1.06) x 0.637
HIP 96948 -8.8 -0.003 +0.06 +0.097 1.04 9.62 C 2.30 1.52 a 0.577
HIP 97420 +32.3 +0.002 +0.04 +0.064 1.01 9.65 B 2.84 2.22 a 0.497
HIP 100963 -1.6 -0.026 -0.02 -0.012 1.00 9.71 A 2.70 1.72 a 0.146
HIP 112504 -16.0 -0.064 -0.01 +0.020 1.02 9.63 C 2.40 2.01 a 0.289
Note. The $\Delta $ values are the parameter differences (relative to the Sun) for $T_{\rm eff}$ (K), $\log g$ (dex), $v_{\rm t}$ (km s-1), and {Fe/H} (dex), which were derived as results from the complete differential analysis (Sect. 3.1.2). The units of the other quantities are as follows: M (in $M_{\odot}$), age (in yr), $v_{\rm r+m}$ (in km s-1), $A_{\rm Li}$ (with the normalization of $A_{\rm H} = 12.00$). See the text for more details regarding the age-reliability class (Qage; Sect. 3.3), the grade of $A_{\rm Li}$-determination ( ${q}_{\rm Li}$; Sect. 4.3), and the relative-to-Sun similarity index ($\sigma$; Appendix A).

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