\begin{table}
\caption{\label{Tab:A}Table of the most polarizing atomic spectral lines of the second 
solar spectrum (3160~\AA$-$6995~\AA). 
The lines are listed by increasing wavelength.
The various quantities that are listed for each line are described in 
Sect.~\ref{sect:tabA}.} 
\begin{tabular}{llccclllll}
\hline\hline\noalign{\smallskip}
\# & $\lambda^{\rm Sun}$ & Elem. & W$_{\lambda}$ & W$_{\lambda}$/$\lambda$ & $(Q/I)^{\rm M}$ & $(Q/I)^{\rm m}$ & $Q/I$ & Type & Notes \\
 & (\AA) & & (m\AA) & (F) & $\;$ (\%) & $\;$ (\%) & (\%) & & \\
\noalign{\smallskip}
\hline
\multicolumn{9}{c}{------------------------------ Volume III ------------------------------} \\
\noalign{\smallskip}
1 & 3179.342 & Ca~{\sc ii} & 580 & 182 & 0.85 & 0.50 & 0.35 & W & 
$^1$ \\
\noalign{\smallskip}
2 & 3217.935 & Ti~{\sc i} & 35 & 11.1 & 0.75 & 0.60$^{\ast}$ & 0.15 & S$^{\ast}$ & 
$^2$ \\
\noalign{\smallskip}
3 & 3230.592 & Sm~{\sc ii} & 34 & 10.5 & 0.86 & 0.65$^{\ast}$ & 0.21 & S$^{\ast}$ & 
$^3$ \\
\noalign{\smallskip} 
4 & 3234.518 & Ti~{\sc ii} & 49 & 15.2 & 0.62 & 0.50 & 0.12 & M1 & 
$^4$ \\
 & & & & & {\it 1.35} & {\it 0.85} & {\it 0.50} & & \\
\noalign{\smallskip} 
5 & 3242.007 & Ti~{\sc ii} & 270 & 83.0 & 0.95 & 0.80 & 0.15 & M1 & \\
 & & & & & {\it 1.07} & {\it 0.84} & {\it 0.23} & & \\
\noalign{\smallskip}
6 & 3247.569 & Cu~{\sc i} & 246 & 76.0 & {\it 1.75} & {\it 0.82} & {\it 0.93} & M0 & 
$^5$ \\
\noalign{\smallskip} 
7 & 3248.612 & /Ti~{\sc ii}  Ti~{\sc i} & 148 & 46.0 & 0.57 & 0.40 & 0.17 & W & 
$^6$ \\
\noalign{\smallskip} 
8 & 3260.552 & Nb~{\sc ii} & 20 & 6.1 & 0.85 & 0.70$^{\ast}$ & 0.15 & S & \\
\noalign{\smallskip} 
9 & 3273.052 & Zr~{\sc ii} & 78 & 23.9 & 0.77 & 0.58 & 0.19 & W & \\
\noalign{\smallskip} 
10 & 3273.972 & Cu~{\sc i} & 221$^{\ast}$ & 67.4 & 0.36 & 0.19 & 0.17 & W & 
$^7$ \\
\noalign{\smallskip} 
11 & 3308.399 & Ti~{\sc i} & 32 & 9.7 & 0.92 & 0.58$^{\ast}$ & 0.34 & S & \\
\noalign{\smallskip} 
12 & 3322.949 & Ti~{\sc ii}  (Zr~{\sc ii}) & 495$^{\ast}$ & 157.3 & 0.42 & 0.27 & 0.15 & M1 & 
$^8$ \\
 & & & & & {\it 0.75} & {\it 0.64} & {\it 0.11} & & \\
\noalign{\smallskip} 
13 & 3326.777 & //Ti~{\sc ii}$-$Zr~{\sc ii} & 214 & 64.0 & 0.275 & 0.175 & 0.100 & W & \\
\noalign{\smallskip} 
14 & 3372.812 & Ti~{\sc ii} & 459 & 135.9 & {\it 0.67} & {\it 0.55} & {\it 0.12} & M0 & \\
\noalign{\smallskip} 
15 & 3380.260 & Ti~{\sc ii} & 30 & 31.2 & 0.25 & 0.15 & 0.10 & W & 
$^9$ \\
\noalign{\smallskip} 
16 & 3380.585 & Ni~{\sc i} & 809 & 239 & 0.275 & 0.175 & 0.100 & W & $^{9}$ \\
\noalign{\smallskip} 
17 & 3383.765 & Ti~{\sc ii} & 430$^{\ast}$ & 127 & {\it 0.65} & {\it 0.53} & {\it 0.12} & M0 & \\
\noalign{\smallskip} 
18 & 3391.973 & Zr~{\sc ii} & 113$^{\ast}$ & 20.0 & 0.42 & 0.32 & 0.10 & W & \\
\noalign{\smallskip} 
19 & 3405.126 & Co~{\sc i} & 206 & 60.5 & {\it 0.67} & {\it 0.49} & {\it 0.18} & M0 & \\
\noalign{\smallskip} 
20 & 3407.805 & Dy~{\sc ii} & 60 & 18.8 & 0.42 & 0.32$^{\ast}$ & 0.10 & S$^{\ast}$ & \\
\noalign{\smallskip} 
21 & 3433.579 & //Ni~{\sc i}$-$Cr~{\sc i} & 492 & 143 & 0.25 & 0.15 & 0.10 & W & \\
\noalign{\smallskip} 
22 & 3439.229 & Gd~{\sc ii} & 10 & 3.5 & 0.53 & 0.40$^{\ast}$ & 0.13 & S & \\
\noalign{\smallskip} 
23 & 3446.271 & Ni~{\sc i} & 470 & 136 & 0.335 & 0.235 & 0.100 & M1 & 
$^{10}$ \\
 & & & & & {\it 0.575} & {\it 0.435} & {\it 0.14} & & \\
\noalign{\smallskip} 
24 & 3452.905 & Ni~{\sc i} & 247 & 73.1 & 0.41 & 0.22 & 0.19 & W & \\
\noalign{\smallskip} 
25 & 3453.512 & Co~{\sc i} & 310 & 87.9 & 0.36 & 0.24 & 0.12 & W & 
$^{11}$ \\
\noalign{\smallskip} 
26 & 3458.467 & Ni~{\sc i} & 656 & 189 & 0.28 & 0.14 & 0.14 & M1 & \\
 & & & & & {\it 0.60} & {\it 0.42} & {\it 0.18} & & \\
\noalign{\smallskip} 
27 & 3461.667 & Ni~{\sc i} & 758 & 219 & 0.33 & 0.16 & 0.17 & W & $^{10}$ \\
\noalign{\smallskip} 
28 & 3464.474 & Sr~{\sc ii}  (Fe~{\sc ii}) & 63 & 18.2 & 0.44 & 0.32$^{\ast}$ & 0.12 & S & \\
\noalign{\smallskip} 
29 & 3465.766 & Co~{\sc i} & 69 & 84.2 & 0.240 & 0.125 & 0.115 & W & 
$^{12}$\\
\noalign{\smallskip} 
30 & 3465.880 & Fe~{\sc i} & 544 & 158 & 0.26 & 0.15 & 0.11 & W & $^{12}$ \\
\noalign{\smallskip} 
31 & 3469.493 & Ni~{\sc i}  (V~{\sc ii}) & 180 & 52.2 & 0.27 & 0.15 & 0.12 & W & \\
\noalign{\smallskip} 
32 & 3472.558 & Ni~{\sc i} & 374 & 136 & 0.31 & 0.175 & 0.135 & W & \\  
\noalign{\smallskip} 
33 & 3476.712 & Fe~{\sc i} & 465 & 136 & 0.34 & 0.19 & 0.15 & W & \\
\noalign{\smallskip} 
34 & 3485.110 & Ni~{\sc i} & 100 & 29.2 & 0.33 & 0.23$^{\ast}$ & 0.10 & S$^{\ast}$ & \\
\noalign{\smallskip} 
35 & 3492.975 & Ni~{\sc i} & 826 & 239 & 0.25 & 0.15 & 0.10 & W & \\
\noalign{\smallskip} 
36 & 3494.515 & /Cr~{\sc ii}  Dy~{\sc ii} & 46 & 13.2 & 0.375 & 0.26$^{\ast}$ & 0.115 & S$^{\ast}$ &
$^{13}$ \\
\noalign{\smallskip} 
37 & 3504.892 & Fe~{\sc i}  /Ti~{\sc ii} & 132 & 37.6 & 0.36 & 0.22 & 0.14 & W & \\
\noalign{\smallskip} 
38 & 3510.846 & Ti~{\sc ii} & 87 & 29.1 & 0.40 & 0.28$^{\ast}$ & 0.12 & S & \\
\noalign{\smallskip} 
39 & 3515.066 & Ni~{\sc i} & 718 & 202 & 0.22 & 0.10 & 0.12 & W & \\
\noalign{\smallskip} 
40 & 3519.618 & Zr~{\sc i} & 7.5 & 2.6 & 0.36 & 0.23$^{\ast}$ & 0.13 & S & \\
\noalign{\smallskip} 
41 & 3521.270 & Fe~{\sc i} & 381 & 110 & 0.24 & 0.11 & 0.13 & W & \\
\noalign{\smallskip} 
42 & 3533.014 & Fe~{\sc i} & 97 & 31.4 & 0.35 & 0.20 & 0.15 & W & 
$^{14}$ \\ 
\noalign{\smallskip} 
43 & 3550.222 & $-$Dy~{\sc ii} & 43 & 12.0 & 0.42 & 0.31 & 0.11 & S & 
$^{15}$\\
\noalign{\smallskip} 
44 & 3553.095 & Pd~{\sc i} & 48$^{\ast}$ & 3.4 & 0.385 & 0.20$^{\ast}$ & 0.185 & S & 
$^{16}$ \\
\noalign{\smallskip} 
45 & 3554.937 & Fe~{\sc i} & 404 & 111 & 0.21 & 0.11 & 0.10 & W & \\
\noalign{\smallskip} 
46 & 3556.597 & Zr~{\sc ii} & 23 & 7.0 & 0.32 & 0.18$^{\ast}$ & 0.14 & S & \\
\noalign{\smallskip} 
47 & 3558.532 & /Fe~{\sc i}$-$Sc~{\sc ii} & 485 & 137 & 0.23 & 0.05 & 0.18 & W & \\
\noalign{\smallskip} 
48 & 3565.396 & Fe~{\sc i} & 990 & 274 & 0.20 & 0.08 & 0.12 & W & 
$^{17}$ \\
\noalign{\smallskip} 
49 & 3566.383 & Ni~{\sc i} & 458 & 141 & 0.32 & 0.22 & 0.10 & M1 & $^{17}$ \\
 & & & & & {\it 0.38} & {\it 0.30} & {\it 0.08} & & \\
\noalign{\smallskip} 
50 & 3570.134 & Fe~{\sc i} & 1380 & 387 & 0.34 & 0.20 & 0.14 & M1 & \\
 & & & & & {\it 0.41} & {\it 0.29} & {\it 0.12} & & \\
\noalign{\smallskip} 
51 & 3578.693 & Cr~{\sc i} & 488 & 142 & 0.42 & 0.17 & 0.25 & M1 & \\
 & & & & & {\it 0.435} & {\it 0.285} & {\it 0.150} & & \\
\noalign{\smallskip} 
52 & 3581.209 & Fe~{\sc i} & 2144 & 599 & 0.34 & 0.18 & 0.16 & M1 & \\
 & & & & & {\it 0.41} & {\it 0.28} & {\it 0.13} & & \\
\noalign{\smallskip} 
53 & 3585.714 & Fe~{\sc i} & 168 & 63.0 & 0.22 & 0.11 & 0.11 & W & 
$^{18}$\\
\noalign{\smallskip} 
54 & 3585.844 & Co~{\sc i}?$-$Ti~{\sc i} & 25 & 22.6 & 0.40 & 0.26$^{\ast}$ & 0.14 & S & $^{18}$ \\
\noalign{\smallskip} 
55 & 3586.990 & Fe~{\sc i} & 532 & 147 & 0.22 & 0.09 & 0.13 & W & \\
\noalign{\smallskip} 
56 & 3589.222 & Ru~{\sc i} & 18 & 5.7 & 0.375 & 0.275 & 0.100 & S & \\
\noalign{\smallskip} 
57 & 3590.489 & Sc~{\sc ii} & 136 & 37.9 & 0.21 & 0.05 & 0.16 & M1 & 
$^{19}$ \\
 & & & & & {\it 0.375} & {\it 0.275} & {\it 0.100} & & \\
\noalign{\smallskip} 
58 & 3592.027 & V~{\sc ii} & 75 & 21.0 & 0.20 & 0.10 & 0.10 & W & \\
\noalign{\smallskip} 
59 & 3593.495 & Cr~{\sc i} & 436 & 127 & 0.775 & 0.270 & 0.505 & M1 & \\
 & & & & & {\it 0.95} & {\it 0.27} & {\it 0.68} & & \\
\noalign{\smallskip} 
60 & 3594.638 & Fe~{\sc i} & 146 & 40.8 & 0.30 & 0.17 & 0.13 & W & \\
\noalign{\smallskip} 
61 & 3594.876 & Co~{\sc i} & 92 & 25.7 & 0.25 & 0.14 & 0.11 & W & \\
\noalign{\smallskip} 
62 & 3596.054 & Ti~{\sc ii} & 95 & 26.7 & 0.21 & 0.07 & 0.14 & W & 
$^{20}$ \\
\noalign{\smallskip} 
63 & 3597.712 & Ni~{\sc i} & 181 & 50.2 & 0.29 & 0.12 & 0.17 & M1 & 
$^{21}$ \\
 & & & & & {\it 0.36} & {\it 0.27} & {\it 0.09} & & \\
\noalign{\smallskip} 
64 & 3600.739 & Y~{\sc ii} & 69 & 19.2 & 0.35 & 0.25 & 0.10 & W & 
$^{22}$ \\
\noalign{\smallskip} 
65 & 3601.198 & Zr~{\sc i} & 13 & 3.6 & 0.42 & 0.31$^{\ast}$ & 0.11 & S & \\
\noalign{\smallskip}
66 & 3602.287 & Ni~{\sc i} & 94 & 26.2 & 0.18 & 0.06 & 0.12 & W & \\
\noalign{\smallskip} 
67 & 3605.339 & //Cr~{\sc i}  Co~{\sc i} & 495 & 136 & 0.24 & 0.09 & 0.15 & W & \\
\noalign{\smallskip}
68 & 3608.869 & Fe~{\sc i} & 1046 & 287 & 0.31 & 0.18 & 0.13 & M1 & \\
 & & & & & {\it 0.44} & {\it 0.26} & {\it 0.18} & & \\
\noalign{\smallskip} 
69 & 3610.166 & //Fe~{\sc i}  Ti~{\sc i} & 231 & 65.4 & 0.26 & 0.11 & 0.15 & W & \\
\noalign{\smallskip} 
70 & 3610.460 & Ni~{\sc i} & 250$^{\ast}$ & 52.0 & 0.27 & 0.08 & 0.19 & W & \\
\noalign{\smallskip} 
71 & 3618.777 & Fe~{\sc i} & 1410 & 385 & 0.39 & 0.15 & 0.24 & M1 & 
$^{23}$ \\
 & & & & & {\it 0.35} & {\it 0.25} & {\it 0.10} & & \\
\noalign{\smallskip} 
72 & 3619.400 & Ni~{\sc i} & 568 & 204 & 0.30 & 0.16 & 0.14 & W & \\
\noalign{\smallskip} 
73 & 3621.467 & Fe~{\sc i} & 140 & 40.6 & 0.19 & 0.09 & 0.10 & W & \\
\noalign{\smallskip} 
74 & 3624.733 & Ni~{\sc i} & 132 & 37.1 & 0.165 & 0.04 & 0.125 & W & \\
\noalign{\smallskip} 
75 & 3631.475 & //Fe~{\sc i}  Cr~{\sc ii} & 1364 & 369 & 0.21 & 0.11 & 0.10 & M1 & \\
 & & & & & {\it 0.31} & {\it 0.24} & {\it 0.07} & & \\
\noalign{\smallskip} 
76 & 3633.138 & Y~{\sc ii} & 134$^{\ast}$ & 19.0 & 0.51 & 0.24 & 0.27 & S & \\
\noalign{\smallskip} 
77 & 3647.851 & Fe~{\sc i}  (Fe~{\sc i}) & 970 & 313 & 0.28 & 0.11 & 0.17 & M1 & \\
 & & & & & {\it 0.31} & {\it 0.23} & {\it 0.08} & & \\
\noalign{\smallskip} 
78 & 3651.800 & Sc~{\sc ii} & 114 & 39.1 & 0.14 & 0.04 & 0.10 & W & \\
\noalign{\smallskip} 
79 & 3664.097 & Ni~{\sc i} & 130 & 43.8 & 0.19 & 0.08 & 0.11 & W & \\
\noalign{\smallskip}
80 & 3674.150 & Ni~{\sc i} & 178$^{\ast}$ & 33.0 & 0.16 & 0.06 & 0.10 & W & \\
\noalign{\smallskip} 
81 & 3694.817 & Dy~{\sc ii} & 24 & 9.2 & 0.30 & 0.20$^{\ast}$ & 0.10 & S & \\
\noalign{\smallskip} 
82 & 3705.577 & Fe~{\sc i} & 562 & 180 & 0.15 & 0.05 & 0.10 & W & \\
\noalign{\smallskip} 
83 & 3710.292 & Y~{\sc ii} & 74 & 27.2 & 0.40 & 0.25$^{\ast}$ & 0.15 & S & \\
\noalign{\smallskip} 
84 & 3719.947 & Fe~{\sc i} & 1664 & 538 & {\it 0.34} & {\it 0.24} & {\it 0.10} & M0 & 
$^{24}$ \\
\noalign{\smallskip} 
85 & 3724.574 & Ti~{\sc i} & 60 & 23.1 & 0.475 & 0.320 & 0.155 & S & \\
\noalign{\smallskip} 
86 & 3728.042 & Ru~{\sc i} & 40 & 20.0 & 0.30 & 0.20$^{\ast}$ & 0.10 & S$^{\ast}$ & 
$^{25}$ \\
\noalign{\smallskip} 
87 & 3733.841 & Cr~{\sc i}? & 2 & 2.3 & 0.57 & 0.42 & 0.15 & S & 
$^{26}$ \\
\noalign{\smallskip} 
88 & 3734.874 & Fe~{\sc i} & 3027 & 945 & 0.480 & 0.275 & 0.205 & W & 
$^{27}$ \\
\noalign{\smallskip} 
89 & 3737.141 & Fe~{\sc i} & 1071 & 428 & 0.31 & 0.16 & 0.15 & W & \\
\noalign{\smallskip} 
90 & 3741.312 & Sm~{\sc ii}$-$Eu~{\sc ii} & 13 & 5.0 & 0.57 & 0.38$^{\ast}$ & 0.19 & S & 
$^{28}$ \\ 
\noalign{\smallskip} 
91 & 3742.278 & Ru~{\sc i} & 6 & 2.4 & 0.50 & 0.375$^{\ast}$ & 0.125 & S & \\
\noalign{\smallskip} 
92 & 3743.368 & Fe~{\sc i} & 592 & 193 & 0.275 & 0.175 & 0.100 & W & \\
\noalign{\smallskip} 
93 & 3745.574 & Fe~{\sc i} & 1202$^{\ast}$ & 459 & 0.325 & 0.200 & 0.125 & W & \\
\noalign{\smallskip} 
94 & 3745.910 & Fe~{\sc i}  (Zr~{\sc ii}) & 540 & 301 & 0.575 & 0.280$^{\ast}$ & 0.295 & S & 
$^{29}$ \\
\noalign{\smallskip} 
95 & 3748.271 & Fe~{\sc i} & 497 & 228 & 0.32 & 0.18 & 0.14 & W & \\
\noalign{\smallskip} 
96 & 3748.966 & /Fe~{\sc i}  Cr~{\sc i} & 103 & 82.9 & 0.275 & 0.175 & 0.100 & W & \\
\noalign{\smallskip} 
97 & 3749.495 & Fe~{\sc i} & 1907 & 578 & 0.45 & 0.20 & 0.25 & W & \\
\noalign{\smallskip} 
98 & 3753.620 & /Fe~{\sc i}$-$Ti~{\sc i} & 132 & 45.0 & 0.16 & 0.30 & 0.14 & W &
$^{30}$ \\
\noalign{\smallskip} 
99 & 3758.245 & Fe~{\sc i} & 1647 & 497 & 0.40 & 0.22 & 0.18 & M1 & \\ 
 & & & & & {\it 0.69} & {\it 0.42} & {\it 0.27} & & \\ 
\noalign{\smallskip} 
100 & 3759.299 & Ti~{\sc ii} & 334 & 115 & 0.41 & 0.31 & 0.10 & W & 
$^{31}$ \\
\noalign{\smallskip} 
101 & 3761.320 & Ti~{\sc ii} & 277$^{\ast}$ & 61.0 & 0.48 & 0.38 & 0.10 & M1 & \\
 & & & & & {\it 0.70} & {\it 0.41} & {\it 0.29} & & \\
\noalign{\smallskip} 
102 & 3763.803 & Fe~{\sc i} & 829 & 255 & 0.36 & 0.15 & 0.21 & M1 & 
$^{32}$ \\
 & & & & & {\it 0.72} & {\it 0.40} & {\it 0.32} & & \\
\noalign{\smallskip} 
103 & 3767.204 & Fe~{\sc i} & 820 & 262 & 0.28 & 0.18 & 0.10 & M1 & \\
 & & & & & {\it 0.55} & {\it 0.40} & {\it 0.15} & & \\
\noalign{\smallskip} 
104 & 3780.516 & /CN$-$Zr~{\sc i} & 26 & 9.5 & 0.51 & 0.39 & 0.12 & S & 
$^{33}$\\
\noalign{\smallskip} 
105 & 3782.318 & CN  /Y~{\sc ii} & 18 & 6.3 & 0.485 & 0.385 & 0.100 & S & \\
\noalign{\smallskip} 
106 & 3784.252 & Nd~{\sc ii}$-$Fe~{\sc i}~p & 16 & 5.8 & 0.65 & 0.38 & 0.27 & S & 
$^{34}$ \\
\noalign{\smallskip} 
107 & 3787.236 & V~{\sc ii}  CN & 139$^{\ast}$ & 17.2 & 0.50 & 0.38 & 0.12 & S & \\
\noalign{\smallskip} 
108 & 3788.861 & /Cr~{\sc i}$-$CN & 69$^{\ast}$ & 17.4 & 0.59 & 0.38 & 0.21 & S & \\
\noalign{\smallskip} 
109 & 3791.194 & CN  Nb~{\sc i} & 8.5 & 3.2 & 0.50 & 0.38 & 0.12 & S & \\
\noalign{\smallskip} 
110 & 3792.565 & /CN  Y~{\sc ii} & 33 & 15.0 & 0.67 & 0.38 & 0.29 & S & \\
\noalign{\smallskip} 
111 & 3796.974 & CN  Cr~{\sc i} & 20 & 16.1 & 0.540 & 0.375 & 0.165 & S & \\
\noalign{\smallskip} 
112 & 3801.371 & Fe~{\sc i}$-$CN & 75 & 30.2 & 0.550 & 0.375 & 0.175 & S & \\
\noalign{\smallskip} 
113 & 3801.542 & Ce~{\sc ii}  CN & 50 & 21.0 & 0.575 & 0.375 & 0.200 & S & \\
\noalign{\smallskip} 
114 & 3806.375 & CN  Fe~{\sc i} & 67 & 22.0 & 0.63 & 0.37 & 0.26 & S & \\
\noalign{\smallskip} 
115 & 3807.937 & /Cr~{\sc i}$-$CN & 111 & 35.2 & 0.52 & 0.39$^{\ast}$ & 0.13 & S & 
$^{35}$ \\ 
\noalign{\smallskip} 
116 & 3809.162 & Fe~{\sc i} & 24 & 9.5 & 0.62 & 0.37 & 0.25 & S & 
$^{36}$ \\
\noalign{\smallskip} 
117 & 3811.380 & CN  Ti~{\sc i}? & 35 & 16.0 & 0.64 & 0.37 & 0.27 & S & \\
\noalign{\smallskip} 
118 & 3812.199 & CN  Y~{\sc ii} & 44$^{\ast}$ & 4.5 & 0.51 & 0.37 & 0.14 & S & \\
\noalign{\smallskip} 
119 & 3813.491 & V~{\sc i} & 54 & 28.4 & 0.49 & 0.36 & 0.13 & S & 
$^{37}$ \\
\noalign{\smallskip} 
120 & 3814.892 & CN  Ti~{\sc i} & 26 & 15.7 & 0.58 & 0.36 & 0.22 & S & \\ 
\noalign{\smallskip} 
121 & 3817.843 & V~{\sc i}  CN  Cr~{\sc i} & 40 & 16.0 & 0.50 & 0.36 & 0.14 & S & \\
\noalign{\smallskip} 
122 & 3824.750 & CN  Fe~{\sc i}~p & 11 & 10.5 & 0.31 & 0.20$^{\ast}$ & 0.11 & S$^{\ast}$ & \\
\noalign{\smallskip} 
123 & 3826.770 & CN$-$V~{\sc i}  Ni~{\sc i} & 15 & 11.2 & 0.48 & 0.35 & 0.13 & S & \\
\noalign{\smallskip} 
124 & 3826.957 & CN$-$/V~{\sc ii} & 32 & 21.7 & 0.47 & 0.35 & 0.12 & S & \\ 
\noalign{\smallskip} 
125 & 3829.365 & Mg~{\sc i} & 874 & 308 & 0.50 & 0.26 & 0.24 & M1 & 
$^{38}$ \\
\noalign{\smallskip} 
126 & 3830.311 & CN?  Sm~{\sc ii} & 7.5 & 3.8 & 0.49 & 0.35 & 0.14 & S & 
$^{39}$ \\
\noalign{\smallskip} 
127 & 3832.310 & Mg~{\sc i} & 1685 & 600 & 0.225 & 0.10 & 0.125 & M1 & $^{38}$ \\
\noalign{\smallskip} 
128 & 3838.302 & Mg~{\sc i} & 1920 & 641 & 0.27 & 0.16 & 0.11 & M1 & $^{38}$ \\
\noalign{\smallskip} 
129 & 3846.986 & CN$-$Zr~{\sc i} & 110$^{\ast}$ & 9.6 & 0.435 & 0.335 & 0.10 & S & \\
\noalign{\smallskip} 
130 & 3848.611 & CN  Ce~{\sc ii} & 41 & 13.5 & 0.470 & 0.335 & 0.135 & S & 
$^{40}$ \\
\noalign{\smallskip} 
131 & 3851.172 & V~{\sc i}  CN & 24 & 9.6 & 0.50 & 0.335 & 0.165 & S & \\
\noalign{\smallskip} 
132 & 3851.599 & CN  Fe~{\sc i} & 13 & 6.1 & 0.565 & 0.330 & 0.235 & S & \\
\noalign{\smallskip} 
133 & 3867.863 & CN  Ru~{\sc i} & 100$^{\ast}$ & 1.6 & 0.500 & 0.325 & 0.175 & S & \\
\noalign{\smallskip} 
134 & 3869.313 & Ti~{\sc i}$-$CN & 120$^{\ast}$ & 22.5 & 0.475 & 0.320 & 0.155 & S & \\
\noalign{\smallskip} 
135 & 3870.552 & CN  Co~{\sc i} & 74$^{\ast}$ & 19.4 & 0.435 & 0.320 & 0.115 & S & \\
\noalign{\smallskip} 
136 & 3871.136 & CN  V~{\sc i}? & 13 & 18.8 & 0.45 & 0.32 & 0.13 & S & \\
\noalign{\smallskip} 
137 & 3872.179 & CN  Fe~{\sc i}? & 19 & 12.4 & 0.525 & 0.320 & 0.205 & S & $^{40}$ \\
\noalign{\smallskip} 
138 & 3883.639 & Cr~{\sc i} & 26 & 9.3 & 0.67 & 0.44$^{\ast}$ & 0.23 & S & \\
\noalign{\smallskip} 
139 & 3891.781 & Ba~{\sc ii} & 30 & 11.6 & 0.54 & 0.40$^{\ast}$ & 0.14 & S & \\
\noalign{\smallskip} 
\multicolumn{9}{c}{------------------------------ Volume II ------------------------------} & 
$^{41}$ \\
\noalign{\smallskip} 
140 & 3920.269 & Fe~{\sc i} & 341 & 101 & 0.50 & 0.15 & 0.35 & W & \\
\noalign{\smallskip} 
141 & 3922.923 & Fe~{\sc i} & 414 & 124 & 0.72 & 0.20 & 0.52 & W & 
$^{42}$ \\
\noalign{\smallskip} 
142 & 3927.933 & Fe~{\sc i}  (CH) & 187 & 144 & 0.51 & 0.10 & 0.41 & W & \\
\noalign{\smallskip} 
143 & 3933.682 & Ca~{\sc ii} [K] & 20~253 & 4874 & 0.80 & 0.00 & 0.80 & M1 & 
$^{43}$ \\
\noalign{\smallskip} 
144 & 3987.966 & Yb~{\sc i} & 18 & 5.0 & 0.53 & 0.42$^{\ast}$ & 0.11 & S & \\
\noalign{\smallskip} 
145 & 4030.763 & Mn~{\sc i} & 326$^{\ast}$ & 75.2 & 0.28 & 0.05 & 0.23 & W & 
$^{44}$ \\
\noalign{\smallskip} 
146 & 4033.072 & Mn~{\sc i} & 229$^{\ast}$ & 54.8 & 0.16 & 0.05 & 0.11 & W & 
$^{44}$ \\
\noalign{\smallskip} 
147 & 4034.492 & Mn~{\sc i} & 213$^{\ast}$ & 46.1 & 0.27 & 0.10 & 0.17 & W & \\
\noalign{\smallskip} 
148 & 4039.096 & Cr~{\sc i} & 42 & 10.4 & 0.445 & 0.345 & 0.100 & S & \\
\noalign{\smallskip} 
149 & 4040.790 & Ce~{\sc ii}$-$Nd~{\sc ii} & 39 & 9.6 & 0.48 & 0.345 & 0.135 & S & 
$^{45}$ \\ 
\noalign{\smallskip} 
150 & 4045.825 & Fe~{\sc i} & 1174 & 316 & 0.465 & 0.190 & 0.275 & M1 & \\
 & & & & & {\it 0.73} & {\it 0.34} & {\it 0.39} & & \\
\noalign{\smallskip} 
151 & 4049.862 & Gd~{\sc ii}  /Fe~{\sc i} & 11 & 2.7 & 0.67 & 0.44$^{\ast}$ & 0.23 & S & \\
\noalign{\smallskip} 
152 & 4062.232 & Ce~{\sc ii} & 6 & 1.5 & 0.49 & 0.33 & 0.16 & S & \\
\noalign{\smallskip} 
153 & 4063.605 & Fe~{\sc i}  (Mn~{\sc i}) & 787 & 219 & 0.34 & 0.08 & 0.26 & M1 & \\
 & & & & & {\it 0.50} & {\it 0.33} & {\it 0.17} & & \\
\noalign{\smallskip} 
154 & 4071.749 & Fe~{\sc i} & 723 & 191 & 0.41 & 0.16 & 0.25 & M1 & 
$^{46}$ \\
 & & & & & {\it 0.63} & {\it 0.32} & {\it 0.31} & & \\
\noalign{\smallskip} 
155 & 4077.724 & Sr~{\sc ii} & 428$^{\ast}$ & 100 & 1.225 & 0.320 & 0.905 & MS & \\
 & & & & & {\it 1.10} & {\it 0.32} & {\it 0.78} & & \\
\noalign{\smallskip} 
156 & 4083.226 & Ce~{\sc ii} & 26 & 6.4 & 0.47 & 0.32 & 0.15 & S & \\
\noalign{\smallskip} 
157 & 4109.450 & Nd~{\sc ii} & 39 & 9.5 & 0.42 & 0.30 & 0.12 & S & \\
\noalign{\smallskip} 
158 & 4115.376 & Ce~{\sc ii} & 11 & 2.7 & 0.430 & 0.295 & 0.135 & S & \\
\noalign{\smallskip} 
159 & 4128.309 & Y~{\sc i} & 12 & 2.9 & 0.595 & 0.290 & 0.305 & S & \\
\noalign{\smallskip}
160 & 4129.724 & Eu~{\sc ii} & 54 & 12.1 & 0.465 & 0.285 & 0.180 & S & \\
\noalign{\smallskip}
161 & 4130.657 & Ba~{\sc ii} & 45 & 10.9 & 0.53 & 0.26$^{\ast}$ & 0.27 & S & 
$^{47}$ \\
\noalign{\smallskip}
162 & 4142.842 & Y~{\sc i} & 22 & 5.3 & 0.445 & 0.280 & 0.165 & S & \\
\noalign{\smallskip}
163 & 4186.126 & Ti~{\sc i} & 42 & 10.0 & 0.53 & 0.27$^{\ast}$ & 0.26 & S & \\
\noalign{\smallskip}
164 & 4222.602 & Ce~{\sc ii} & 22 & 5.2 & 0.42 & 0.30$^{\ast}$ & 0.12 & S & \\
\noalign{\smallskip}
165 & 4226.740 & Ca~{\sc i} & 1476 & 342 & 2.190 & 0.235 & 1.955 & M1 & \\
 & & & & & {\it 2.700} & {\it 0.235} & {\it 2.465} & & \\
\noalign{\smallskip}
166 & 4233.612 & Fe~{\sc i} & 298 & 70.4 & 0.14 & 0.24 & 0.10 & W & 
$^{48}$ \\
\noalign{\smallskip}
167 & 4235.949 & Fe~{\sc i}  (Cr~{\sc i})  (Y~{\sc i}) & 385 & 90.9 & 0.12 & 0.27 & 0.15 & W & 
$^{49}$ \\
\noalign{\smallskip}
168 & 4237.891 & Ti~{\sc i} & 16 & 4.0 & 0.38 & 0.23 & 0.15 & S & \\
\noalign{\smallskip}
169 & 4246.837 & Sc~{\sc ii} & 171 & 40.3 & 0.460 & 0.225 & 0.235 & MS & 
$^{50}$ \\
 & & & & & {\it 0.470} & {\it 0.225} & {\it 0.245} & & \\
\noalign{\smallskip}
170 & 4250.130 & Fe~{\sc i} & 342$^{\ast}$ & 79.5 & 0.26 & 0.12 & 0.14 & W & \\
\noalign{\smallskip}
171 & 4254.346 & Cr~{\sc i}  (V~{\sc ii}) & 393 & 92.4 & 0.40 & 0.16 & 0.24 & M1 & \\
 & & & & & {\it 0.270} & {\it 0.225} & {\it 0.045} & & \\
\noalign{\smallskip}
172 & 4268.628 & V~{\sc i} & 23 & 5.6 & 0.45 & 0.22 & 0.23 & S & \\
\noalign{\smallskip}
173 & 4271.774 & Fe~{\sc i} & 756 & 177 & 0.24 & 0.09 & 0.15 & W & \\
\noalign{\smallskip}
174 & 4274.806 & Cr~{\sc i} & 196 & 45.8 & 0.59 & 0.22 & 0.37 & M1 & \\
 & & & & & {\it 0.36} & {\it 0.22} & {\it 0.14} & & \\
\noalign{\smallskip}
175 & 4283.014 & Ca~{\sc i} & 133 & 31.0 & 0.33 & 0.18 & 0.15 & W & 
$^{51}$ \\
\noalign{\smallskip}
176 & 4289.922 & Fe~{\sc i}  (Ce~{\sc ii}) & 65 & 19.1 & 0.285 & 0.170 & 0.115 & S & \\
\noalign{\smallskip}
177 & 4299.249 & /Fe~{\sc i}  Ti~{\sc i}  (CH) & 212 & 49.3 & 0.22 & 0.12 & 0.10 & W & 
$^{52}$ \\
%
\noalign{\smallskip}
178 & 4307.748 & Ca~{\sc i} & 59 & 40.2 & 0.14 & 0.04 & 0.10 & S & 
$^{53}$ \\
\noalign{\smallskip}
179 & 4307.912 & /Fe~{\sc i}  Ti~{\sc ii}  (CH) & 723 & 165 & 0.14 & 0.04 & 0.10 & W & 
$^{54}$ \\
\noalign{\smallskip}
180 & 4325.775 & Fe~{\sc i}  (Fe~{\sc i} p) & 793 & 174 & 0.32 & 0.12 & 0.20 & M1 & \\
 & & & & & {\it 0.380} & {\it 0.195} & {\it 0.185} & & \\
\noalign{\smallskip}
181 & 4339.722 & Cr~{\sc i} & 69 & 23.8 & 0.27 & 0.15$^{\ast}$ & 0.12 & S & \\
\noalign{\smallskip}
182 & 4340.475 & H~{\sc i} [H$_{\gamma}$] & 2855 & 659 & 0.25 & 0.13 & 0.12 & W & \\
\noalign{\smallskip}
183 & 4354.436 & La~{\sc ii} & 13 & 3.4 & 0.295 & 0.195$^{\ast}$ & 0.100 & S & 
$^{55}$ \\
\noalign{\smallskip}
184 & 4374.944 & Y~{\sc ii} & 88 & 20.1 & 0.39 & 0.18 & 0.21 & S & \\
\noalign{\smallskip}
185 & 4383.557 & Fe~{\sc i} & 1008 & 235 & 0.410 & 0.110 & 0.300 & M1 &
$^{56}$ \\
 & & & & & {\it 0.305} & {\it 0.175} & {\it 0.130} & & \\
\noalign{\smallskip}
186 & 4404.761 & Fe~{\sc i} & 898 & 181 & 0.29 & 0.06 & 0.23 & M1 & \\
 & & & & & {\it 0.23} & {\it 0.17} & {\it 0.06} & & \\
\noalign{\smallskip}
187 & 4415.135 & Fe~{\sc i} & 417$^{\ast}$ & 92.9 & 0.07 & 0.20 & 0.13 & W & \\
\noalign{\smallskip}
188 & 4425.444 & Ca~{\sc i} & 145 & 31.6 & 0.275 & 0.165 & 0.110 & S & \\
\noalign{\smallskip}
189 & 4431.292 & Ti~{\sc i} & 5 & 1.1 & 0.38 & 0.16 & 0.22 & S & 
$^{57}$ \\
\noalign{\smallskip}
190 & 4453.710 & Ti~{\sc i} & 36 & 9.0 & 0.280 & 0.155 & 0.125 & S & \\
\noalign{\smallskip}
191 & 4460.225 & Ce~{\sc ii} & 100$^{\ast}$ & 6.0 & 0.315 & 0.155 & 0.160 & S & 
$^{58}$ \\
\noalign{\smallskip}
192 & 4462.993 & Nd~{\sc ii} & 13 & 2.9 & 0.26 & 0.15 & 0.11 & S & \\
\noalign{\smallskip}
193 & 4471.244 & Ti~{\sc i}  (Ce~{\sc ii}) & 35 & 8.5 & 0.265 & 0.165$^{\ast}$ & 0.100 & S & \\
\noalign{\smallskip}
194 & 4486.914 & Ce~{\sc ii} & 11 & 2.5 & 0.28 & 0.15 & 0.13 & S & \\
\noalign{\smallskip}
195 & 4500.288 & Cr~{\sc i} & 39$^{\ast}$ & 6.2 & 0.230 & 0.145 & 0.085 & S & \\
\noalign{\smallskip} 
196 & 4511.900 & Cr~{\sc i} & 31 & 8.4 & 0.180 & 0.125$^{\ast}$ & 0.055 & S & \\
\noalign{\smallskip} 
197 & 4527.325 & //Ti~{\sc i}  /Cr~{\sc i}  (Ce~{\sc ii}) & 67 & 14.8 & 0.210 & 0.140 & 0.070 & S & \\
\noalign{\smallskip} 
198 & 4536.054 & Ti~{\sc i} & 147$^{\ast}$ & 16.3 & 0.240 & 0.125$^{\ast}$ & 0.115 & S & \\
\noalign{\smallskip}
199 & 4540.710 & Cr~{\sc i} & 52 & 12.3 & 0.165 & 0.110$^{\ast}$ & 0.055 & S & \\
\noalign{\smallskip} 
200 & 4554.036 & Ba~{\sc ii} & 159 & 36.7 & 0.78 & 0.13 & 0.65 & MS & \\
 & & & & & {\it 0.50} & {\it 0.13} & {\it 0.37} & & \\
\noalign{\smallskip}
201 & 4572.284 & Ce~{\sc ii} & 15 & 3.3 & 0.205 & 0.130 & 0.075 & S & \\
\noalign{\smallskip} 
202 & 4595.593 & Cr~{\sc i} & 21 & 4.6 & 0.255 & 0.105$^{\ast}$ & 0.150 & S & \\
\noalign{\smallskip}
203 & 4599.227 & Ti~{\sc i} & 6 & 1.3 & 0.185 & 0.120 & 0.065 & S & \\
\noalign{\smallskip} 
204 & 4607.338 & Sr~{\sc i} & 36 & 7.8 & 1.200 & 0.120 & 1.080 & S & \\
\noalign{\smallskip}
\multicolumn{9}{c}{------------------------------ Volume I ------------------------------} & 
$^{59}$ \\
\noalign{\smallskip}
205 & 4639.368 & Ti~{\sc i} & 36 & 8.4 & 0.185 & 0.115 & 0.070 & S & \\
\noalign{\smallskip} 
206 & 4639.946 & Ti~{\sc i} & 31 & 7.3 & 0.175 & 0.115 & 0.060 & S & \\
\noalign{\smallskip} 
207 & 4679.983 & Fe~{\sc i} p & 6.5 & 1.4 & 0.155 & 0.105 & 0.050 & S & \\
\noalign{\smallskip} 
208 & 4703.003 & Mg~{\sc i} & 326 & 71.9 & 0.095 & 0.045 & 0.050 & W & \\
\noalign{\smallskip} 
209 & 4742.798 & Ti~{\sc i} & 27 & 5.7 & 0.290 & 0.098 & 0.192 & S & \\
\noalign{\smallskip}
210 & 4758.124 & Ti~{\sc i} & 40 & 8.2 & 0.202 & 0.095 & 0.107 & S & \\
\noalign{\smallskip}
211 & 4759.276 & Ti~{\sc i} & 41 & 8.6 & 0.192 & 0.095 & 0.097 & S & \\
\noalign{\smallskip}
212 & 4778.258 & Ti~{\sc i} & 16 & 3.3 & 0.148 & 0.092 & 0.056 & S & \\
\noalign{\smallskip} 
213 & 4796.189 & Cr~{\sc i}$-$//Ti~{\sc i} & 24 & 5.0 & 0.145 & 0.090 & 0.055 & S & \\
\noalign{\smallskip} 
214 & 4799.794 & V~{\sc i}$-$//Ti~{\sc i} & 75$^{\ast}$ & 10.2 & 0.175 & 0.089 & 0.086 & S & \\
\noalign{\smallskip} 
215 & 4805.420 & Ti~{\sc i} & 37 & 7.7 & 0.150 & 0.087 & 0.063 & S & \\
\noalign{\smallskip} 
216 & 4840.884 & Ti~{\sc i} & 60 & 12.6 & 0.136 & 0.082 & 0.054 & S & 
$^{60}$ \\
\noalign{\smallskip} 
217 & 4868.263 & Ti~{\sc i} & 26 & 5.5 & 0.130 & 0.080 & 0.050 & S & \\
\noalign{\smallskip} 
218 & 4975.351 & Ti~{\sc i} & 35$^{\ast}$ & 3.6 & 0.165 & 0.070 & 0.095 & S & 
$^{61}$ \\
\noalign{\smallskip} 
219 & 5021.923 & Cr~{\sc i}  Fe~{\sc i}  C2 & 22 & 4.4 & 0.115 & 0.065 & 0.050 & S & \\
\noalign{\smallskip} 
220 & 5025.764 & Fe~{\sc i}  C2 & 11 & 2.2 & 0.124 & 0.063 & 0.061 & S & \\
\noalign{\smallskip} 
221 & 5112.279 & Zr~{\sc ii} & 8 & 1.6 & 0.106 & 0.056 & 0.050 & S & \\
\noalign{\smallskip} 
222 & 5113.127 & /Cr~{\sc i}  MgH & 23 & 4.5 & 0.120 & 0.056 & 0.064 & S & \\
\noalign{\smallskip} 
223 & 5115.790 & Fe~{\sc i} & 23 & 4.5 & 0.120 & 0.056 & 0.064 & S & 
$^{62}$ \\
\noalign{\smallskip} 
224 & 5120.420 & Ti~{\sc i} & 31 & 6.0 & 0.135 & 0.055 & 0.080 & S & 
$^{63}$ \\
\noalign{\smallskip} 
225 & 5138.717 & Cr~{\sc i}$-$MgH & 13 & 2.4 & 0.130 & 0.055 & 0.075 & S & \\
\noalign{\smallskip} 
226 & 5139.648 & Cr~{\sc i} & 46 & 8.9 & 0.120 & 0.054 & 0.066 & S & 
$^{64}$ \\
\noalign{\smallskip}
227 & 5146.119 & Fe~{\sc ii}~p  C2 & 37 & 6.6 & 0.140 & 0.054 & 0.086 & S & 
$^{65}$ \\
\noalign{\smallskip} 
228 & 5149.796 & Co~{\sc i}  MgH & 11 & 2.1 & 0.126 & 0.053 & 0.073 & S & \\
\noalign{\smallskip} 
229 & 5153.241 & Cu~{\sc i} & 56$^{\ast}$ & 8.5 & 0.163 & 0.053 & 0.110 & S & 
$^{66}$ \\
\noalign{\smallskip}
230 & 5167.327 & Mg~{\sc i} & 935$^{\ast}$ & 173 & 0.130 & 0.030 & 0.100 & W & \\
\noalign{\smallskip}
231 & 5171.028 & Ru~{\sc i}  MgH & 5 & 1.0 & 0.110 & 0.052 & 0.058 & S & \\
\noalign{\smallskip} 
232 & 5176.792 & /V~{\sc i}$-$MgH & 10 & 1.9 & 0.115 & 0.051 & 0.064 & S & \\
\noalign{\smallskip} 
233 & 5196.452 & Cr~{\sc i} & 34 & 6.5 & 0.090 & 0.040$^{\ast}$ & 0.050 & S & 
$^{67}$ \\
\noalign{\smallskip} 
234 & 5206.044 & Cr~{\sc i}  (Ti~{\sc i}) & 216$^{\ast}$ & 36.6 & 0.115 & 0.050 & 0.065 & MS & 
$^{68}$ \\
 & & & & & {\it 0.115} & {\it 0.050} & {\it 0.065} & & \\
\noalign{\smallskip} 
235 & 5208.432 & Cr~{\sc i} & 247 & 47.4 & 0.110 & 0.040 & 0.070 & MS & $^{68}$ \\
 & & & & & {\it 0.077} & {\it 0.050} & {\it 0.027} & & \\
\noalign{\smallskip} 
236 & 5218.209 & Cu~{\sc i} & 48 & 9.8 & 0.101 & 0.049 & 0.052 & S & \\
\noalign{\smallskip} 
237 & 5239.823 & Sc~{\sc ii} & 55 & 10.5 & 0.117 & 0.048 & 0.069 & S & \\
\noalign{\smallskip} 
238 & 5387.565 & Cr~{\sc i} & 25$^{\ast}$ & 1.8 & 0.100 & 0.040 & 0.060 & S & 
$^{69}$ \\
\noalign{\smallskip}
239 & 5528.418 & Mg~{\sc i} & 293 & 53.8 & 0.052 & 0.000 & 0.052 & W & \\
\noalign{\smallskip}
240 & 5535.51 & Ba~{\sc i} & 113$^{\ast}$ & & 0.165 & 0.032 & 0.133 & S & \\
\noalign{\smallskip}
241 & 5565.485 & Ti~{\sc i} & 16 & 2.9 & 0.150 & 0.031 & 0.119 & S & \\
\noalign{\smallskip}
242 & 5598.491 & Ca~{\sc i} & 118 & 21.1 & 0.080 & 0.030 & 0.050 & S & \\
\noalign{\smallskip} 
243 & 5644.146 & Ti~{\sc i} & 29 & 5.1 & 0.260 & 0.029 & 0.231 & S & \\
\noalign{\smallskip}
244 & 5889.973 & Na~{\sc i} [D$_{2}$] & 752$^{\ast}$ & 120 & 0.330 & 0.021 & 0.309 & MS & \\
 & & & & & {\it 0.220} & {\it 0.021} & {\it 0.199} & & \\
\noalign{\smallskip}
245 & 5895.940 & Na~{\sc i} [D$_{1}$] & 564$^{\ast}$ & 91.0 & 0.05 & --0.02 & 0.07 & $-$ & 
$^{70}$ \\
\noalign{\smallskip}
246 & 6024.068 & Fe~{\sc i} & 117$^{\ast}$ & 19.8 & 0.060 & 0.010$^{\ast}$ & 0.050 & S & \\
\noalign{\smallskip}
247 & 6141.727 & /Ba~{\sc ii}$-$Fe~{\sc i} & 113 & 19.4 & 0.059 & 0.000 & 0.059 & W & \\
\noalign{\smallskip}
248 & 6562.808 & H~{\sc i} [H$_{\alpha}$] & 4020 & 649 & 0.120 & 0.010 & 0.110 & S & $^{71}$\\
\hline
\end{tabular} 
\smallskip 
$^{1}$ The linear polarization signal is quite noisy at this wavelength, and 
it is not possible to measure the amplitude of the $Q/I$ profile with high 
precision. There are four more lines in this spectral region that, 
although showing linear polarization peaks with amplitudes apparently larger 
than~0.1\%, have not been included in this table because of the high noise 
level: Fe~{\sc i} at 3171.665~\AA, //Fe~{\sc i} at 3172.051~\AA, Cr~{\sc ii} 
Fe~{\sc i}~p (CH) at 3172.087~\AA, and Fe~{\sc i} at 3180.236~\AA.\\
$^{2}$ The polarization peak does not fall exactly at line center. 
This could be due to the fact that the line is severely blended with a 
depolarizing Ni~{\sc i}~line at 3217.841~\AA, which may imply also a reduction 
of the peak amplitude.\\
$^{3}$ This signal is a typical case where it is not easy to establish the 
reference level from which the amplitude of the $Q/I$ peak has to be 
measured.\\
$^{4}$ This signal has been associated with the Ti~{\sc ii} line since the 
$Q/I$ central peak falls at the wavelength position of the line-core of this 
spectral line, and because it is very similar to the signal produced by the 
Ti~{\sc ii} line at 3242.007~\AA, which belongs to the same multiplet. 
However, the strong polarization signal in the wings may be
produced by the combined action of this line and of the nearby line at 
3234.647~{\AA} (Ni~{\sc i}$-$Fe~{\sc i}).\\
$^{5}$ This is a very deep line in the intensity spectrum, and unavoidably 
the polarization signal is rather noisy at line center. For this reason it is 
not easy to determine if it has to be classified as ``M0''~or ``M1''.
The polarization lobe in the blue wing of the line is almost completely 
destroyed by the presence of depolarizing blended lines.\\
$^{6}$ The ``W''~shape of this signal 
might be due to the effect of depolarizing lines blended with the red and blue 
wings of this spectral line.\\
$^{7}$ The polarization peak does not fall exactly at line center. 
This displacement, as well as the large width of the intensity 
profile of this line, could be explained by the presence of a blend with an
OH line, or in terms of the hyperfine structure shown by this element.\\
$^{8}$ The depolarization observed beside the line-core peak of this line 
might be affected by the presence of blended lines. Moreover, it is not 
possible to exclude that the polarization observed in the far wings could be 
affected (or due) to the NH band. In this latter case the signal should be 
classified as ``W''.\\
$^{9}$ These lines are severely blended. 
The larger reduced equivalent width of the Ni~{\sc i} line suggests that the 
broad depolarization is due to this line, while the Ti~{\sc ii} line produces 
a much narrower ``W''~signal. \\
$^{10}$ The polarization peak at line center shows a substructure made of 
two secondary peaks separated by a small dip. \\
$^{11}$ It is not possible to exclude that this signal might be of type 
``M1'', the wing-peaks being hidden by blended lines.\\
$^{12}$ These lines are severely blended, and it is difficult to understand 
if they are both ``W'', or if only one is ``W'', the other one being ``S''. 
\\
$^{13}$ The polarization peak does not fall exactly at line center.\\
$^{14}$ This line falls in the blue depolarizing wing of a Fe~{\sc i} line, 
and it is not easy to determine if this signal has to be classified as ``S''~
or ``W''.\\
$^{15}$ The polarization peak has quite a large width. This could be due to 
the unidentified blended line, or to the hyperfine structure shown by this 
element. This second hypothesis is supported by the similarity with the 
polarization signal of the Dy~{\sc ii} line at 3407.805~\AA.\\ 
$^{16}$ It is not easy to establish the reference level from which the 
amplitude of the $Q/I$ peak has to be measured.\\
$^{17}$ It is not possible to exclude that the polarization peak at 
3566.7~\AA$\;$ could be due to the interferences between the Fe~{\sc i} lines 
at 3565.396~\AA$\;$ and 3570.134~\AA, which belong to the same multiplet. 
In this case the Fe~{\sc i} signal should be classified as ``M1''~instead of 
``W'', while the Ni~{\sc i} signal as~``W''~instead of ``M1''.\\
$^{18}$ The width of the polarization peak at the wavelength position of the 
Co~{\sc i}$-$Ti~{\sc i} line (line \# 54) is a little surprising. 
It is not possible to exclude that this peak might pertain to a possible ``M1''~
structure of the Fe~{\sc i} line at 3585.714~\AA. 
In this case, the Co~{\sc i}$-$Ti~{\sc i} line should be excluded. 
\\ 
$^{19}$ In the blue wing of this line the polarization might be enhanced by 
(or due to) the presence of a blending Fe~{\sc i} line at 3590.302~\AA, in the 
red wing it could be affected by the wing-lobe of the far, strong Cr~{\sc i} 
line at 3593.495~\AA. It is difficult, therefore, to determine if this line 
should be classified as ``M1'', or ``W''.\\
$^{20}$ Very likely the polarization in the blue wing is due to the strong 
Cr~{\sc i} line at 3593.495~\AA, while in the red wing to the Ni~{\sc i} line 
at 3597.712~\AA. If this is not the case, the signal should be classified as 
``M1''.\\
$^{21}$ It is not possible to exclude that the polarization in the far wings 
of this line might be the wing-lobes of the far Cr~{\sc i} line at 
3593.495~\AA. In this case the signal should be classified as ``W''.\\
$^{22}$ The polarization lobes in the far wings do not seem to be due to this 
line. If this is not the case, the signal should be classified as ``M1''.\\
$^{23}$ We have classified this signal as ``M1'', since its wing-lobes appear 
to be severely blended by several depolarizing lines.\\
$^{24}$ This line produces a very broad polarization signal. The 
amplitude of the wing-lobes has been measured in the blue wing at 
3717.0~\AA.\\
$^{25}$ The polarization peak does not fall exactly at line center, being 
slightly shifted to the blue.\\
$^{26}$ This polarization signal, though being located at the wavelength 
position corresponding to a (possible) Cr~{\sc i} line, might be due either to 
CN or to the strong, nearby Fe~{\sc i} line at 3734.874~\AA.\\
$^{27}$ It is not possible to exclude that the signal at 3733.841~{\AA} 
(\# 87) might be due to this Fe~{\sc i} line. In this case this signal 
should be classified as ``M1''~instead of ``W''.\\
$^{28}$ The polarization peak does not fall exactly at line center, being 
slightly shifted to the blue. This may indicate that the signal is due 
to Sm~{\sc ii}.\\
$^{29}$ This signal falls in the depolarizing wing of the broad Fe~{\sc i} 
line at 3745.574~\AA$~$ (belonging to the same multiplet), and it is 
difficult to determine if this is a ``S''~or a ``W''~signal.\\
$^{30}$ The dip in the red wing, which is free of blends, induces to believe 
that this is a ``W''~signal, the dip in the blue wing being missing because of 
the blend with the Dy~{\sc ii}$-$CN line at 3753.525~\AA.\\
$^{31}$ This signal falls in the strongly polarized red wing of the 
Fe~{\sc i} line at 3758.245~\AA, and it is not possible to exclude that it 
might be classified as an ``M''~signal. Note that the Ti~{\sc ii} line at 
3761.320~\AA$~$ (classified as ``M1'') belongs to the same multiplet.\\
$^{32}$ The amplitude of the wing-lobe might be enhanced by the presence of 
CN lines.\\
$^{33}$ The polarization peak does not fall exactly at line center, but it 
is slightly shifted to the blue. This may be an indication that the signal is 
due to~CN.\\
$^{34}$ Given the extremely low value of the Einstein coefficient of the 
Fe~{\sc i} line ($2\times10^3$~s$^{-1}$), it seems quite reasonable to 
believe that this signal is produced by the Nd~{\sc ii} line.\\
$^{35}$ The polarization peak does not fall exactly at line center, but it 
is slightly red-shifted. This is a strong hint that this signal might be due 
to CN.\\
$^{36}$ The polarization peak does not seem to be as sharp as for an isolated 
line. Probably there is a contribution coming from the CN molecule.\\
$^{37}$ The width of this polarization signal suggests that it might be 
enhanced by (or due to) the strongly blending Ti~{\sc ii} line at 3813.394~\AA. 
It is not possible to exclude therefore that the Ti~{\sc ii} line should be 
included in the table, and classified as ``M0''.\\
$^{38}$ The wing-lobes of these lines are probably heavily affected 
(enhanced) by several CN lines. For this reason the wing-lobe amplitudes have 
not been measured. \\
$^{39}$ The polarization signal is severely blended with other CN lines.\\
$^{40}$ The polarization peak does not fall exactly at line center, but is 
somewhat red-shifted. \\
$^{41}$ Volume~III of the atlas covers the spectral interval between 
3160~{\AA} and 3915~{\AA}, Vol.~II the spectral interval between 3910~{\AA} 
and 4630~{\AA}. The spectral interval between 3910.0~{\AA} and 3913.5~{\AA} is 
covered by both volumes. Comparing the observations made in this spectral
interval, it can be noticed that the theoretical continuum plotted in Vol.~III 
is slightly lower than in Vol.~II, while the peaks observed in $Q/I$ in 
Vol.~III are slightly larger than 
in Vol.~II. This might be due to the fact that,
although the nominal position of the slit is $\mu=0.1$ for the observations of 
both atlases, because of the seeing the ``effective''~position
might be different from the nominal value.\\
$^{42}$ At line center this signal shows quite a complex profile, with 
several secondary peaks and dips.\\
$^{43}$ At line center the Ca~{\sc ii} K line shows a ``M''~type profile, 
but it is important to note that quantum interferences between the 
Ca~{\sc ii} H and K~lines produce a much broader signal that starts in the far 
blue wing of the K line, at about 3890~\AA, with a positive lobe. 
The polarization becomes negative between the K and H lines, and it is zero 
(without showing any particular structure) at the wavelength position of the 
H line. This structure 
(which does not enter the classification scheme proposed in this work) has 
already been explained in terms of quantum interferences by \citet{Ste80a} 
and \citet{LL04}. It is quite surprising, however, that the
atlas does not show any positive lobe in the red wing of the Ca~{\sc ii} H 
line, predicted on the other hand by  the theory. This might be due to the 
choice of the level of the local polarized continuum, which may be wrong 
between 3972~\AA$~$ and 3990~\AA. Note that where the polarization is 
negative, a depolarizing line produces a $Q/I$ peak. For this reason, all the 
lines producing polarization peaks in this spectral interval have not been 
included in the table.
Note also that three lines (Sc~{\sc i}, V~{\sc i} and Co~{\sc i}), falling 
within an interval of $\approx$ 0.5~{\AA} centered at the core of the 
Ca~{\sc ii} K line, are listed as masked lines by \citet{Moore66}. \\
$^{44}$ At line center this signal shows quite a complex profile with 
several secondary peaks and dips, perhaps due to hyperfine structure.
\\
$^{45}$ The polarization signal is slightly blue-shifted with respect to 
line center.\\
$^{46}$ At line center this signal shows quite a complex profile with 
several secondary peaks and dips.\\
$^{47}$ This line is severely blended with a weaker Ce~{\sc ii} line. 
In the absence of this blend, the amplitude of $Q/I$ peak might be 
different.\\
$^{48}$ At line center this signal shows quite a complex profile with 
several secondary peaks and dips.\\
$^{49}$ It is not possible to exclude that the ``W''~shape of this signal 
could be due to the depolarization produced by several blending lines.\\
$^{50}$ The polarization profile shows a complex structure (that might be 
due to hyperfine structure), and an extended blue wing.\\
$^{51}$ The depolarization in the blue wing of this profile is rather 
peculiar. For this reason the reference level for measuring the signal 
amplitude has been taken in the dip of the red wing.\\
$^{52}$ It is difficult to measure the amplitude of this signal because of 
the presence of several blends.\\
$^{53}$ It is difficult to decide whether this line has to be classified as 
``S''~or ``W''~because of the blend with the /Fe~{\sc i} Ti~{\sc i} (CH) line 
at 4307.912~\AA, and because the polarization signal is quite noisy around this 
wavelength.\\
$^{54}$ At line center this line shows a two-peak structure, probably 
due to the blend.\\
$^{55}$ The polarization peak does not fall exactly at line center, probably 
because of the presence of a strong blend with a Mg~{\sc i} line. 
It is not possible to exclude that in the absence of this blend, the $Q/I$ 
peak amplitude would have been significantly larger.\\
$^{56}$ At line center this line shows a complex structure, with several 
secondary peaks and dips.\\
$^{57}$ This line is severely blended with a Sc~{\sc ii} line. 
In the absence of this blend the amplitude of the $Q/I$ signal might be
larger.\\
$^{58}$ This line is severely blended with a V~{\sc i} line. In the absence 
of this blend the amplitude of the $Q/I$ signal might be larger.\\
$^{59}$ Volume~II of the atlas covers the spectral interval between 
3910~{\AA} and 4630~{\AA}, Vol.~I the spectral interval between 4625~{\AA} 
and 6995~{\AA}. The spectral interval between 4624~{\AA} and 4626.5~{\AA} is 
covered by both volumes. Comparing the observations made in this spectral
interval, it can be noticed that the depolarization produced by two rather 
intense lines (Fe~{\sc i} and Cr~{\sc i}) is larger in Vol.~I than in Vol.~II. 
As already discussed in the note 41, this might be due to the 
fact that, although the nominal position of the slit is $\mu=0.1$ for the 
observations of both atlases, because of the seeing the 
``effective''~position might be different from the nominal value.\\
$^{60}$ A secondary peak is observed to the blue of line center. The 
observation in this spectral region is quite noisy, and at this level it is 
not possible to exclude that the signal could be of ``W''~type.\\
$^{61}$ This line is severely blended with a Fe~{\sc i} line. 
In the absence of this blend the amplitude of the $Q/I$ signal might be 
larger.\\
$^{62}$ This line has an extremely weak Einstein coefficient 
(5.15$\times$10$^{4}$~s$^{-1}$), and it is not possible to exclude that this 
polarization signal might be due to a C$_2$ line.\\
$^{63}$ The polarization peak does not fall exactly at line center, 
probably because of the presence of a strong blend with a Fe~{\sc ii}~p 
C$_2$ line. It is not possible to exclude that in the absence of this blend, 
the $Q/I$ peak amplitude would have been larger.\\
$^{64}$ This line is severely blended with a Fe~{\sc i} line. 
In the absence of this blend the amplitude of the $Q/I$ signal might be 
larger.\\
$^{65}$ This polarization signal is quite wide. This may be due to the 
presence of a blending C$_2$ line.\\
$^{66}$ The large width of this polarization profile, and the fact that the 
peak does not fall at line center, suggest that the 
blending C$_2$ line might affect significantly this signal.\\
$^{67}$ The signal is somewhat noisy in this spectral region, and it is not 
possible to exclude that the signal might be classified as ``W''.\\
$^{68}$ Very likely the overall structure of the polarization signal in the 
interval between 5204~{\AA} and 5210~{\AA} is due to quantum interferences 
between the $J$-levels of the term $^5$P$^{\rm o}$. Both lines seem to show 
an ``MS''~structure partially hidden by blends. \\
$^{69}$ This line is severely blended with a Fe~{\sc i} line.
In the absence of this blend the amplitude of the $Q/I$ signal might be 
larger.\\
$^{70}$ This signal cannot be classified according to the scheme proposed 
in this work.\\
$^{71}$ According to our scheme, this polarization signal has to be 
classified as ``S''. However, it has to be remarked that its width is much 
larger than the width of any other signal of this class.
\end{table}