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Table A.11

Stellar parameters for the whole sample, Fe differential abundance (Δ[Fe/H]), and the resulting membership based on the abundance homogeneity criterium.

Name Instrumenta T eff log g ξ log ϵ(Fe i) log ϵ(Fe ii) [Fe/H] Δ[Fe/H] M(Fe)b Tot.c M d
HD 115043 H, T 5941 ± 30 4.60 ± 0.08 1.22 ± 0.04 7.46 ± 0.02 7.45 ± 0.04 −0.010 ± 0.005 – ± – Y 20 Y
HD 4048 T 6428 ± 77 4.56 ± 0.17 1.15 ± 0.10 7.56 ± 0.06 7.56 ± 0.07 0.080 ± 0.011 0.089 ± 0.010 Y 13 N
V445 And F, T 6028 ± 38 4.62 ± 0.09 1.20 ± 0.06 7.44 ± 0.03 7.45 ± 0.04 −0.030 ± 0.006 −0.012 ± 0.005 Y 20 Y
HD 8004 T 6072 ± 38 4.58 ± 0.10 0.95 ± 0.06 7.50 ± 0.03 7.50 ± 0.04 0.029 ± 0.006 0.040 ± 0.006 Y 19 Y*
HD 13829 T 6158 ± 62 4.49 ± 0.14 0.83 ± 0.09 7.55 ± 0.05 7.54 ± 0.06 0.045 ± 0.008 0.055 ± 0.008 Y 20 Y
HD 20367 T 6107 ± 38 4.49 ± 0.09 1.02 ± 0.05 7.59 ± 0.03 7.59 ± 0.04 0.108 ± 0.006 0.118 ± 0.006 Y 18 Y*
γ Lep A H 6441 ± 38 4.72 ± 0.11 1.67 ± 0.06 7.43 ± 0.03 7.42 ± 0.05 −0.039 ± 0.006 −0.039 ± 0.006 Y 19 Y*
γ Lep B H 4907 ± 55 4.39 ± 0.15 0.71 ± 0.19 7.35 ± 0.03 7.35 ± 0.09 −0.112 ± 0.007 −0.112 ± 0.007 Y 18 Y*
V1386 Ori H 5292 ± 23 4.52 ± 0.06 0.98 ± 0.05 7.43 ± 0.02 7.44 ± 0.03 −0.026 ± 0.004 −0.022 ± 0.004 Y 19 Y*
HD 51419 T 5662 ± 25 4.32 ± 0.07 0.86 ± 0.04 7.10 ± 0.02 7.10 ± 0.03 −0.371 ± 0.004 −0.364 ± 0.005 N 0 N
HD 56168 H 5044 ± 35 4.53 ± 0.10 0.81 ± 0.09 7.28 ± 0.02 7.28 ± 0.06 −0.175 ± 0.005 −0.169 ± 0.006 N 9 N
DX Lyn H 5073 ± 37 4.44 ± 0.10 0.80 ± 0.10 7.38 ± 0.02 7.38 ± 0.06 −0.073 ± 0.005 −0.069 ± 0.005 Y 20 Y
V869 Mon F, T 5007 ± 65 4.52 ± 0.20 1.09 ± 0.15 7.38 ± 0.04 7.38 ± 0.13 −0.089 ± 0.008 −0.080 ± 0.010 Y 19 Y*
HD 64942 F 5869 ± 36 4.63 ± 0.09 1.11 ± 0.06 7.48 ± 0.03 7.48 ± 0.04 0.011 ± 0.005 0.025 ± 0.005 Y 20 Y
HD 72659 H 5956 ± 14 4.30 ± 0.04 1.21 ± 0.02 7.46 ± 0.01 7.47 ± 0.02 0.001 ± 0.003 0.009 ± 0.003 Y 16 N
II Cnc H 5409 ± 24 4.49 ± 0.06 0.99 ± 0.04 7.43 ± 0.02 7.43 ± 0.03 −0.030 ± 0.004 −0.022 ± 0.004 Y 20 Y
HD 76218 H 5376 ± 25 4.47 ± 0.08 0.97 ± 0.05 7.41 ± 0.02 7.40 ± 0.04 −0.053 ± 0.004 −0.044 ± 0.004 Y 19 Y*
HD 81659 H 5706 ± 19 4.48 ± 0.05 0.99 ± 0.03 7.63 ± 0.01 7.63 ± 0.02 0.168 ± 0.003 0.175 ± 0.004 N 9 N
HD 91148 H 5637 ± 21 4.43 ± 0.05 0.90 ± 0.03 7.55 ± 0.02 7.55 ± 0.02 0.095 ± 0.003 0.103 ± 0.003 Y 20 Y
HD 91204 H 5945 ± 17 4.37 ± 0.06 1.20 ± 0.02 7.68 ± 0.01 7.68 ± 0.03 0.225 ± 0.003 0.231 ± 0.003 N 4 N
HD 93215 H 5822 ± 17 4.46 ± 0.05 1.06 ± 0.02 7.68 ± 0.01 7.68 ± 0.02 0.224 ± 0.003 0.229 ± 0.003 N 5 N
HD 100310 F 5459 ± 26 4.48 ± 0.07 0.74 ± 0.05 7.33 ± 0.02 7.33 ± 0.04 −0.137 ± 0.004 −0.124 ± 0.005 N 8 N
HD 104289 H 6301 ± 32 4.48 ± 0.06 1.38 ± 0.04 7.58 ± 0.02 7.58 ± 0.03 0.113 ± 0.005 0.128 ± 0.004 Y 19 Y*
DO CVn F 5015 ± 65 4.61 ± 0.17 1.05 ± 0.16 7.38 ± 0.03 7.39 ± 0.11 −0.078 ± 0.008 −0.072 ± 0.008 Y 20 Y
NP UMa F 4997 ± 59 4.60 ± 0.17 1.16 ± 0.16 7.34 ± 0.03 7.34 ± 0.11 −0.126 ± 0.008 −0.115 ± 0.008 N 17 N
HD 116497 H 6222 ± 27 4.61 ± 0.06 1.24 ± 0.03 7.56 ± 0.02 7.56 ± 0.03 0.099 ± 0.004 0.111 ± 0.003 Y 20 Y
HN Boo H, T 4990 ± 63 4.47 ± 0.19 1.08 ± 0.17 7.45 ± 0.04 7.45 ± 0.12 −0.001 ± 0.010 0.002 ± 0.008 Y 19 Y*
HP Boo F 6072 ± 26 4.59 ± 0.06 1.27 ± 0.04 7.51 ± 0.02 7.51 ± 0.03 0.042 ± 0.003 0.060 ± 0.003 Y 20 Y
ξ Boo F, T 5513 ± 26 4.57 ± 0.08 1.14 ± 0.04 7.31 ± 0.02 7.31 ± 0.04 −0.162 ± 0.004 −0.155 ± 0.012 N 4 N
HD 135143 H 6094 ± 18 4.55 ± 0.05 1.14 ± 0.03 7.56 ± 0.01 7.56 ± 0.02 0.103 ± 0.003 0.111 ± 0.003 Y 20 Y
AN CrB F 5106 ± 44 4.56 ± 0.13 1.04 ± 0.10 7.27 ± 0.03 7.27 ± 0.08 −0.197 ± 0.005 −0.185 ± 0.006 N 8 N
HD 150706 H, F, T 5953 ± 25 4.57 ± 0.08 1.13 ± 0.04 7.43 ± 0.02 7.43 ± 0.03 −0.036 ± 0.004 −0.028 ± 0.005 Y 20 Y
HD 151044 F 6203 ± 21 4.54 ± 0.05 1.32 ± 0.03 7.51 ± 0.02 7.51 ± 0.02 0.042 ± 0.003 0.059 ± 0.003 Y 20 Y
HD 153458 H 5832 ± 19 4.48 ± 0.05 1.04 ± 0.02 7.56 ± 0.02 7.56 ± 0.02 0.096 ± 0.003 0.104 ± 0.004 Y 19 Y*
HD 153637 H, T 5976 ± 63 4.45 ± 0.14 1.19 ± 0.11 7.19 ± 0.05 7.19 ± 0.06 −0.274 ± 0.010 −0.266 ± 0.003 N 1 N
HD 162209 H 5948 ± 11 4.38 ± 0.04 1.15 ± 0.02 7.56 ± 0.01 7.55 ± 0.02 0.097 ± 0.002 0.105 ± 0.003 Y 15 N
HD 163183 H, T 6083 ± 71 4.72 ± 0.17 1.31 ± 0.11 7.48 ± 0.05 7.48 ± 0.08 0.016 ± 0.010 0.035 ± 0.018 Y 19 Y*
HD 167043 H 6264 ± 25 4.20 ± 0.06 1.72 ± 0.04 7.51 ± 0.02 7.51 ± 0.03 0.049 ± 0.004 0.061 ± 0.004 Y 20 Y
HD 167389 T 5978 ± 20 4.56 ± 0.05 1.17 ± 0.03 7.49 ± 0.02 7.49 ± 0.02 0.011 ± 0.003 0.023 ± 0.004 Y 19 Y*
HD 181655 H 5687 ± 18 4.48 ± 0.04 0.95 ± 0.03 7.51 ± 0.01 7.52 ± 0.02 0.056 ± 0.002 0.064 ± 0.003 Y 20 Y
HD 184385 H 5511 ± 22 4.48 ± 0.06 0.94 ± 0.03 7.51 ± 0.02 7.51 ± 0.03 0.054 ± 0.003 0.058 ± 0.004 Y 20 Y
HD 184960 H, F, T 6446 ± 41 4.57 ± 0.08 1.73 ± 0.06 7.46 ± 0.03 7.47 ± 0.04 −0.006 ± 0.007 0.006 ± 0.014 Y 18 Y*
HD 188015 H 5732 ± 23 4.43 ± 0.06 0.98 ± 0.03 7.69 ± 0.02 7.69 ± 0.03 0.232 ± 0.003 0.238 ± 0.004 N 5 N
HD 216625 T 6320 ± 50 4.58 ± 0.11 1.38 ± 0.07 7.57 ± 0.04 7.57 ± 0.04 0.097 ± 0.007 0.104 ± 0.007 Y 16 N
MT Peg F, T 5944 ± 25 4.57 ± 0.07 1.16 ± 0.03 7.54 ± 0.02 7.54 ± 0.03 0.069 ± 0.004 0.083 ± 0.005 Y 18 Y*

Notes.

(a)

Instruments employed to acquire the data: HERMES (H), FOCES (F), and TLS (T).

(b)

If the star satisfies or not the Fe homogeneity criterium at 1 rms.

(c)

The number of chemical elements satisfying homogeneity at 1 rms.

(d)

If the star satisfies or not the homogeneity criterium in all the analysed elements. Y* means that the remaining 1 or 2 elements satisfy the 1.5 rms criterium but not the 1 rms.

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