Table 6: Abundance ratios derived and atomic parameters adopted.
Species $\lambda$ $\chi_{\rm ex}$ C6 log gf [X/Fe] EW (m${\rm
\AA}$)  
  (${\rm
\AA}$) (eV)   ZOC04 present Arcturus HP1-2 HP1-3 HP1-2 HP1-3
[OI] 6300.311 0.00 0.30E-31 -9.716 -9.716 +0.20 +0.4 +0.4 34.8 33.2  
NaI 6154.230 2.10 0.90E-31 -1.561 -1.56 -0.2 0.0 +0.0 19.0 33.8  
NaI 6160.753 2.10 0.30E-31 -1.261 -1.26 -0.2 0.0 +0.0: 22.0 -  
MgI 6318.720 5.11 0.30E-31 -2.102 -2.10 +0.30 0.0 +0.20 16.2 32.4  
MgI 6319.242 5.11 0.30E-31 -2.362 -2.36 +0.30 0.0 +0.20 12.8 22.6  
MgI 6319.490 5.11 0.30E-31 -2.802 -2.90 +0.30 - +0.20 - 3.6  
MgI 6765.450 5.75 0.30E-31 -1.943 -1.94 +0.30 0.0 +0.20: 7.4 7.1  
SiI 5948.548 5.08 2.19E-30a -1.172 -1.17 +0.25 +0.3 +0.3 80.8 58.2  
SiI 6142.494 5.62 0.30E-31 -1.502 -1.58 +0.25 +0.3 +0.3 22.3 18.7  
SiI 6145.020 5.61 0.30E-31 -1.452 -1.5 +0.25 +0.3 +0.3 21.0 20.0  
SiI 6155.142 5.62 0.30E-30 -0.852 -0.85 +0.35 +0.3 +0.3 53.1 55.4  
SiI 6237.328 5.61 0.30E-30 -1.013 -1.1 +0.25 +0.2 +0.3 29.6 39.0  
SiI 6243.823 5.61 0.30E-32 -1.304 -1.30 +0.25 - +0.2 - 19.7  
SiI 6414.987 5.87 0.30E-30 -1.132 -1.13 +0.35 - +0.3 - 21.7  
SiI 6721.844 5.86 0.90E-30 -1.173 -1.17 +0.25 +0.3 +0.3 23.5 30.5  
CaI 6102.727 1.88 4.54E-31a -0.791 -0.93 +0.25 +0.1 +0.1 137.7 143.8  
CaI 6156.030 2.52 4.0E-31aa -2.392 -2.59 +0.20 -0.1 +0.2 2.3 14.5  
CaI 6161.295 2.51 4.0E-31aa -1.021 -1.42 +0.10 +0.0 +0.1 37.2 -  
CaI 6162.167 1.89 3.0E-31aa -0.091 -0.09 -0.10 +0.0 +0.1 200.0 -  
CaI 6166.440 2.52 3.97E-31aa -0.901 -1.156 +0.20 +0.0 +0.1 78.2 104.2  
CaI 6169.044 2.52 3.97E-31aa -0.541 -0.90 +0.10 +0.0 +0.1 72.6 105.4  
CaI 6169.564 2.52 4.0E-31aa -0.271 -0.63 +0.10 +0.0 +0.1 98.0 -  
CaI 6439.080 2.52 3.4E-32aa +0.34 +0.3 +0.00 +0.0 +0.1: 166.5 -  
CaI 6455.605 2.52 3.39E-32aa -1.351 -1.55 +0.10 +0.0: - 55.2 -  
CaI 6464.679 2.52 3.4E-32aa -2.102 -2.48 +0.40 - - - -  
CaI 6471.668 2.52 3.39E-32aa -0.591 -0.80 +0.00 -0.1 +0.1 74.0 95.6  
CaI 6493.788 2.52 3.37E-32aa +0.141 0.0 -0.15 -0.1 -0.1 141.0 146.9  
CaI 6499.654 2.52 3.37E-32aa -0.591 -0.85 -0.15 -0.1 +0.1 81.0 110.9  
CaI 6508.846 2.52 3.37E-32aa -2.503 -2.51 +0.10 - - - -  
CaI 6572.779 0.00 1.75E-32aa -4.291 -4.32 +0.10 -0.1 +0.1 63.4 111.3  
CaI 6717.687 2.71 4.1E-31aa -0.611 -0.61 +0.10 -0.1 +0.1 - 131.9  
TiI 5866.452 1.07 1.44E-32aa -0.841 -0.84 +0.1 +0.0 +0.0 80.5 109.5  
TiI 5922.110 1.05 2.32E-32aa -1.471 -1.50 +0.1 +0.1 +0.0 56.3 66.8  
TiI 5965.835 1.88 2.14E-32a -0.411 -0.45 +0.1 +0.1 +0.0 48.4 77.3  
TiI 5978.549 1.87 1.43E-32aa -0.501 -0.55 +0.1 +0.1 +0.0 27.4 52.4  
TiI 6064.626 1.05 1.37E-32aa -1.941 -1.94 +0.1 - - - -  
TiI 6091.177 2.27 2.59E-32aa -0.421 -0.42 +0.0 +0.1 +0.0 18.1 45.7  
TiI 6126.224 1.07 1.37E-32aa -1.431 -1.43 +0.0 +0.0 +0.0: 50.0 68.3  
TiI 6258.110 1.44 3.17E-32aa -0.361 -0.36 +0.1 -0.1 +0.0 63.5 113.2  
TiI 6261.106 1.43 4.68E-32a -0.481 -0.48 +0.1 +0.1 +0.0 91.3 120.9  
TiI 6303.767 1.44 3.12E-32aa -1.571 -1.57 +0.1 +0.1 +0.1 16.1 40.6  
TiI 6312.238 1.46 3.17E-32aa -1.691 -1.69 +0.2: +0.1 +0.0 - 31.2  
TiI 6336.113 1.44 1.86E-32aa -1.741 -1.74 +0.1 - +0.1: 22.2 32.8  
TiI 6508.154 1.43 1.46E-32a -2.053 -2.05 +0.1 - +0.0: - 10.9  
TiI 6554.238 1.44 1.81E-32aa -1.221 -1.22 +0.1 -0.1 +0.0 22.7 67.3  
TiI 6556.077 1.46 1.81E-32aa -1.071 -1.07 +0.1 +0.1 +0.0 41.3 68.6  
TiI 6599.113 0.90 1.96E-32aa -2.091 -2.09 +0.1 +0.1 +0.0 20.8 55.1  
TiI 6743.127 0.90 0.30E-31 -1.631 -1.73 +0.1 -0.2 +0.0 32.9 79.7  
TiII 6491.580 2.06 0.30E-31 -2.101* -2.10 +0.1 +0.1 +0.3: 73.2 79.1  
TiII 6559.576 2.05 0.30E-31 -2.483 -2.35 +0.1 - +0.1 - 5.4  
TiII 6606.970 2.06 0.30E-31 -2.791 -2.85 +0.1 +0.1 +0.0 22.9 22.9  
BaII 6141.727 0.70   hfs hfs -0.20 +0.2 +0.2 158.1 162.1  
BaII 6496.908 0.60   hfs hfs -0.20 +0.0 +0.2 192.0 179.6  
LaII 6390.480 0.32   hfs hfs -0.30 0.0 +0.0 18.0 20.3  
EuII 6645.127 1.38   hfs hfs +0.30 +0.0 +0.3 17.4 31.9  
a Damping constants computed following Barklem et al. (1998, 2000); aa damping constants computed as in a, decreased by a factor 1.5 (C6/1.5). Other C6 values are van der Waals classical ones, as described in Zoccali et al. (2004). Column 5 reports the log gf used in Zoccali et al. (2004), adopted from 1 NIST/VALD; 2 Barbuy et al. (1999); 3 McWilliam & Rich (1994); 4 Bensby et al. (2004), whereas Col. 6 gives the values derived in this work from a fit to the solar spectrum; * for TiII 6491.58 ${\rm
\AA}$ line, the NIST log gf = -2.10 is different from the VALD value of log gf = -1.793.


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