Table A.1: Abundances of the light elements.
Mult. $\lambda$(Å) $\log~gf$ Ref.a $\chi_{{\rm low}}$(cm-1) $\log(\gamma_{{\rm S}}/N_{{\rm e}})$ Ref.b W(mÅ) $\log(N_{Z}/N_{\rm tot}$) Notes
He I     $\log N$(He I)/ $N_{\rm tot}$ = -1.73      
88 (22) 3819.6020 -2.968 NIST 169 086.87   DS90   -1.73  
88 (22) 3819.6028 -1.045 NIST 169 086.87   DS90   -1.73  
88 (22) 3819.6028 -1.794 NIST 169 086.87   DS90   -1.73  
88 (22) 3819.6131 -1.794 NIST 169 086.95   DS90   -1.73  
88 (22) 3819.6139 -1.315 NIST 169 086.95   DS90   -1.73  
88 (22) 3819.7573 -1.668 NIST 169 087.93   DS90   -1.73  
82 (20) 3867.4723 -2.055 NIST 169 086.87   DS90   -1.73  
82 (20) 3867.4837 -2.276 NIST 169 086.95   DS90   -1.73  
82 (20) 3867.6315 -2.754 NIST 169 087.93   DS90   -1.73  
32 (58) 3926.5443 -1.647 NIST 171 155.00   DS90   -1.73 Not observed
31 (55) 4009.2565 -1.473 NIST 171 135.00   DS90   -1.73 Not observed
25 (54) 4023.9798 -2.577 NIST 171 135.00   DS90   -1.73 On the wing of He I 4026
87 (18) 4026.1844 -2.625 NIST 169 086.87   SM69   -1.73 Bad fit for the blue wing
87 (18) 4026.1859 -1.448 NIST 169 086.87   SM69   -1.73  
87 (18) 4026.1860 -0.701 NIST 168 086.87   SM69   -1.73  
87 (18) 4026.1968 -1.449 NIST 169 086.95   SM69   -1.73  
87 (18) 4026.1983 -0.972 NIST 169 086.95   SM69   -1.73  
87 (18) 4026.3570 -1.324 NIST 169 087.93   SM69   -1.73  
81 (16) 4120.8108 -1.738 NIST 169 086.87   G74   -1.73 On the red wing of H$\delta$
81 (16) 4120.8237 -1.961 NIST 169 086.95   G74   -1.73  
81 (16) 4120.9916 -2.437 NIST 169 087.93   G74   -1.73  
30 (53) 4143.7590 -1.196 NIST 171 135.00   DS90   -1.73 Not observed
24 (52) 4168.9716 -2.338 NIST 171 135.00   DS90   -1.73 Not observed
29 (51) 4387.9291 -0.883 NIST 171 135.00   SM69   -1.73  
23 (50) 4437.5536 -2.034 NIST 171 135.00   G74   -1.73  
86 (14) 4471.4704 -2.203 NIST 169 086.87   BCS1   -1.73  
86 (14) 4471.4741 -1.026 NIST 169 086.87   BCS1   -1.73  
86 (14) 4471.4743 -0.278 NIST 169 086.87   BCS1   -1.73  
86 (14) 4471.4856 -1.025 NIST 169 086.95   BCS1   -1.73  
86 (14) 4471.4893 -0.550 NIST 169 086.95   BCS1   -1.73  
86 (14) 4471.6832 -0.903 NIST 169 087.93   BCS1   -1.73  
80 (12) 4713.1392 -1.230 NIST 169 086.87   G74   -1.73 Blend with Cr II, Fe II
80 (12) 4713.1562 -1.452 NIST 169 086.94   G74   -1.73  
80 (12) 4713.3757 -1.928 NIST 169 087.93   G74   -1.73  
28 (48) 4921.9310 -0.435 NIST 171 135.00   BCS2   -1.73  
13 ( 4) 5015.6776 -0.820 NIST 166 277.54   G74   -1.73 Blend with Fe II
22 (47) 5047.7384 -1.601 NIST 171 135.00   G74   -1.73 Blend with Fe II
85 (11) 5875.5987 -1.516 NIST 169 086.87   G74   -1.73  
85 (11) 5875.6139 -0.341 NIST 169 086.87   G74   -1.73  
85 (11) 5875.6148 +0.408 NIST 169 086.87   G74   -1.73  
85 (11) 5875.6251 -0.340 NIST 169 086.95   G74   -1.73  
85 (11) 5875.6403 +0.137 NIST 169 086.95   G74   -1.73  
85 (11) 5875.9663 -0.215 NIST 169 087.93   G74   -1.73  
27 (46) 6678.1517 +0.329 NIST 171 135.00   G74   -1.73  
79 (10) 7065.179 -0.461 NIST 169 086.87   G74   -1.73  
79 (10) 7065.217 -0.682 NIST 169 086.95   G74   -1.73  
79 (10) 7065.710 -1.160 NIST 169 087.93   G74   -1.73  
Be II     $\log N$(Be II)/ $N_{\rm tot}$ = -10.64      
1 3130.420 -0.168 K,BIE 0.00 -5.80 G74 (K) 7.12 -10.64  
C I    $\log N$(C I)/ $N_{\rm tot}$ = -4.11 $\pm$ 0.23      
6 4771.747 -1.866 CNO 60 393.14 -4.59 G74 1.58 -3.82  
13 4932.049 -1.658 CNO 61 981.82 -4.32 G74 1.19 -4.05  
3 9062.487 -0.456 CNO 60 333.43 -5.32 G74 24.41 -3.98  
3 9111.807 -0.298 CNO 60 393.14 -5.32 G74 21.88 -4.19  
2 9603.034 -0.896 CNO 60 333.43 -5.40 G74 3.05: -4.49  
C II   $\log N$(C II)/ $N_{\rm tot}$ = -4.05 $\pm$ 0.16      
4 3918.968 -0.533 CNO 131 724.37 -4.93 G74 12.23 -3.95  
6 4267.261 +0.717 CNO 145 550.70 -4.76 G74 22.57 -3.87  
2 6578.052 -0.026 CNO 116 537.65 -5.35 G74 8.68 -4.31 On the wing of H$_{\alpha}$
2 6582.882 -0.328 CNO 116 537.65 -5.35 G74 7.60 -4.08 On the wing of H$_{\alpha}$
O I    $\log N$(O I)/ $N_{\rm tot}$ = -3.18 $\pm$ 0.11      
3 3947.295 -2.096 CNO 73 768.20 -4.70 G74 6.54 -3.40  
3 3947.481 -2.244 CNO 73 768.20 -4.70 G74   -3.40  
3 3947.586 -2.467 CNO 73 768.20 -4.70 G74   -3.40  
5 4368.190 -2.665 CNO 76 794.98 -4.68 G74   -3.20  
5 4368.242 -1.964 CNO 76 794.98 -4.68 G74   -3.20  
5 4368.258 -2.818 CNO 76 794.98 -4.68 G74   -3.20  
14 4967.380 -2.086 CNO 86 625.76 - -     No fit
14 4967.380 -1.997 CNO 86 625.76 - -     No fit
14 4967.380 -2.329 CNO 86 625.76 - -     No fit
14 4967.880 -1.660 CNO 86 627.78 - -     No fit
14 4967.880 -1.865 CNO 86 627.78 - -     No fit
14 4967.880 -2.454 CNO 86 627.78 - -     No fit
14 4968.790 -1.375 CNO 86 631.45 - -     No fit
14 4968.790 -1.961 CNO 86 631.45 - -     No fit
14 4968.790 -2.087 CNO 86 631.45 - -     No fit
13 5020.218 -1.725 CNO 86 631.45 - - 2.87 -3.35  
12 5329.096 -1.938 CNO 86 625.76 -3.43 G74   -3.27  
12 5329.099 -1.586 CNO 86 625.76 -3.43 G74   -3.27  
12 5329.107 -1.695 CNO 86 625.76 -3.43 G74   -3.27  
12 5329.673 -2.063 CNO 86 627.78 -3.43 G74   $\le$-3.27 Blend with Mn II
12 5329.681 -1.473 CNO 86 627.78 -3.43 G74   $\le$-3.27 Blend with Mn II
12 5329.690 -1.269 CNO 86 627.78 -3.43 G74   $\le$-3.27 Blend with Mn II
12 5330.735 -1.570 CNO 86 631.45 -3.43 G74   -3.27  
12 5330.741 -0.984 CNO 86 631.45 -3.43 G74   -3.27  
11 5435.178 -1.766 CNO 86 625.76 -3.82 G74 4.20 -3.20  
11 5435.775 -1.544 CNO 86 627.78 -3.82 G74 5.99 -3.16  
11 5436.862 -1.398 CNO 86 631.45 -3.82 G74 7.49 -3.20  
10 6155.961 -1.363 CNO 86 625.76 -3.96 G74   -3.17  
10 6155.971 -1.011 CNO 86 625.76 -3.96 G74   -3.17  
10 6155.989 -1.120 CNO 86 625.76 -3.96 G74   -3.17  
10 6156.737 -1.488 CNO 86 627.78 -3.96 G74   -3.17  
10 6156.755 -0.899 CNO 86 627.78 -3.96 G74   -3.17  
10 6156.778 -0.694 CNO 86 627.78 -3.96 G74   -3.17  
10 6158.149 -1.841 CNO 86 631.45 -3.96 G74   -3.17 Blend with Cr II, Cr II
10 6158.172 -0.996 CNO 86 631.45 -3.96 G74   -3.17 Blend with Cr II, Cr II
10 6158.187 -0.409 CNO 86 631.45 -3.96 G74   -3.17 Blend with Cr II, Cr II
9 6453.602 -1.288 CNO 86 625.76 -4.28 G74 7.34 -3.24  
9 6454.444 -1.066 CNO 86 627.78 -4.28 G74 11.95 -3.23  
9 6455.977 -0.920 CNO 86 631.45 -4.28 G74   (-3.27) Blend with Ga II
21 7001.899 -1.489 CNO 88 630.59 -3.93 G74   -3.27 Blend with Mn II
21 7001.922 -1.012 CNO 88 630.59 -3.93 G74   -3.27 Blend with Mn II
21 7002.173 -2.644 CNO 88 631.15 -3.93 G74   -3.22  
21 7002.196 -1.489 CNO 88 631.15 -3.93 G74   -3.22  
21 7002.230 -0.741 CNO 88 631.15 -3.93 G74   -3.22  
21 7002.250 -1.364 CNO 88 631.30 -3.93 G74   -3.22  
38 7156.701 +0.288 CNO 102 662.03 -5.35 G74 23.70 -3.11  
1 7771.944 +0.369 CNO 73 768.20 -5.55 G74 190.78 -2.04 No fit
1 7774.166 +0.223 CNO 73 768.20 -5.55 G74 174.48 -2.08 No fit
1 7775.388 +0.001 CNO 73 768.20 -5.55 G74 148.12 -2.20 No fit
35 7947.548 +0.500 K, NBS 101 135.41 -5.54 G74 32.22 -3.02  
35 7950.803 +0.340 K, NBS 101 147.53 -5.54 G74 25.98 -3.09  
35 7952.159 +0.170 K, NBS 101 155.42 -5.54 G74 21.46 -3.14  
34 8221.824 +0.313 CNO 101 135.41 -5.40 G74   -3.10  
4 8446.247 -0.463 CNO 76 794.98 -5.44 G74     No fit
4 8446.359 +0.236 CNO 76 794.98 -5.44 G74     No fit
4 8446.758 +0.014 CNO 76 794.98 -5.44 G74     No fit
37 8820.423 +0.379 CNO 102 662.03 -5.51 G74 43.43 -3.04  
8 9260.806 -0.242 CNO 86 625.76 -4.95 G74     No fit
8 9260.848 +0.110 CNO 86 625.76 -4.95 G74     No fit
8 9260.848 +0.001 CNO 86 625.76 -4.95 G74     No fit
8 9262.582 -0.367 CNO 86 627.78 -4.95 G74     No fit
8 9262.670 +0.223 CNO 86 627.78 -4.95 G74     No fit
8 9262.776 +0.427 CNO 86 627.78 -4.95 G74     No fit
8 9265.826 -0.719 CNO 86 631.45 -4.95 G74     No fit
8 9265.932 +0.126 CNO 86 631.45 -4.95 G74     No fit
8 9266.006 +0.712 CNO 86 631.45 -4.95 G74     No fit
Ne I    $\log N$(Ne I)/ $N_{\rm tot}$ = -4.35    
1 7032.413 -0.294 NIST 134 041.840 -6.32 G74 2.23 -4.35  
Na I    $\log N$(Na I)/ $N_{\rm tot}$ = -5.47    
6 5688.205 -0.450 K, KP 16 973.37 -5.68 G74   -5.47: Blend with telluric lines
1 5889.950 +0.112 NIST 0.00 -5.64 G74   -5.47: Blend interstell./circumstell. line
1 5895.924 -0.191 NIST 0.00 -5.64 G74   -5.47: Blend interstell./ circumstell. line
4 8183.255 +0.260 NIST 16 956.17 -5.52 G74   $\ge $-5.47: Blend with telluric line
4 8194.790 -0.441 NIST 16 973.37 -5.52 G74   -5.47  
4 8194.824 +0.514 NIST 16 973.37 -5.52 G74   -5.47  
Mg I   $\log N$(Mg I)/ $N_{\rm tot}$ = -4.64 $\pm$ 0.06    
40 4702.991 -0.374 NIST 35 051.26 -3.98 G74 2.09 -4.72  
2 5167.321 -0.856 NIST 21 850.41 -5.27 G74 5.80 -4.57  
2 5172.684 -0.380 NIST 21 870.46 -5.27 G74 13.74 -4.63  
2 5183.604 -0.158 NIST 21 911.18 -5.27 G74   -4.58 Blend with Fe II,Ti II
Mg II   $\log N$(Mg II)/ $N_{\rm tot}$ = -4.71 $\pm$ 0.07    
10 4384.637 -0.792 NIST 80 619.50 -4.02 G74 24.11 -4.81  
10 4390.514 -1.706 NIST 80 650.02 -4.02 G74 39.57 -4.76  
10 4390.572 -0.530 NIST 80 650.02 -4.02 G74 39.57 -4.76  
9 4427.994 -1.201 NIST 80 619.50 -4.40 G74 13.44 -4.70  
4 4481.126 +0.730 NIST 71 490.19 -4.68 G74   -4.69 Bad fit for the core
4 4481.150 -0.570 NIST 71 490.19 -4.68 G74   -4.69 Bad fit for the core
4 4481.325 +0.575 NIST 71 490.06 -4.68 G74   -4.69 Bad fit for the core
8 7877.054 +0.390 NIST 80 619.50 -4.54 G74 64.50 -4.68  
8 7896.042 -0.303 NIST 80 650.02 -4.54 G74 28.14 -4.77  
8 7896.366 +0.647 NIST 80 650.02 -4.54 G74 85.58 -4.56 Blend with telluric line
- 8213.987 -0.279 NIST 80 619.50 -4.77 G74   -4.81 At the Paschen limit
- 8234.636 +0.024 NIST 80 650.02 -4.77 G74   -4.81 Blend with telluric line
- 9631.891 +0.663 NIST 93 310.59 - - 57.42 -4.69  
- 9631.95 -0.639 NIST 93 310.59 - -   -4.69  
- 9632.430 +0.507 NIST 93 311.11 - - 47.05 -4.72  
Si II    $\log N$(Si II)/ $N_{\rm tot}$ = -4.72 $\pm$ 0.08    
1 3853.665 -1.517 K, BBCB 55 309.35 -4.91 G74 60.94 -4.77  
1 3856.018 -0.557 K, BBCB 55 325.18 -4.91 G74 108.86 -4.81  
1 3862.595 -0.817 K, BBCB 55 309.35 -4.91 G74 98.75 -4.71  
3.01 4072.709 -2.367 K, SG 79 338.50 -4.51 LDA 1.95 -4.75  
3.01 4075.452 -1.403 K, SG 79 355.02 -4.51 LDA 15.18 -4.72  
7.26 4190.724 -0.351 LA 108 820.60 -5.07 LDA 7.52 -4.66  
7.26 4198.133 -0.611 LA 108 778.70 -5.07 LDA 4.99 -4.59  
5 5041.024 +0.174 NIST 81 191.34 -4.70 G74 73.40 -4.65  
5 5055.984 +0.441 NIST 81 251.32 -4.70 G74 90.48 -4.65  
5 5056.317 -0.535 NIST 81 251.32 -4.70 G74 38.52 -4.63  
7.03 5466.432 -0.190 NIST 101 023.05 -3.85 G74 11.11 -4.74  
7.33 5669.563 +0.266 LA 114 529.14 - - 5.68 -4.75  
7.33 5688.817 +0.106 LA 114 414.58 - - 3.22 -4.87  
4 5957.559 -0.349 NIST 81 191.34 -4.91 G74 37.52 -4.65  
4 5978.930 -0.061 NIST 81 251.32 -4.91 G74 49.34 -4.65  
7.02 7848.816 +0.335 NIST 101 023.05 -4.25 G74 11.81 -4.81  
7.02 7849.722 +0.492 NIST 101 024.35 -4.25 G74 13.41 -4.89  
Si III    $\log N$(Si III)/ $N_{\rm tot}$ = -4.58 $\pm$ 0.04    
2 4552.622 +0.292 NIST 153 377.05 - - 4.01 -4.62  
2 4567.840 +0.069 NIST 153 377.05 - - 3.15 -4.54  
P II   $\log N$(P II)/ $N_{\rm tot}$ = -6.28 $\pm$ 0.08    
7 5296.077 -0.134 K, HI 87 124.60 - - 2.20 -6.33  
6 5316.055 -0.341 K, HI 86 743.96 -4.09 G74 1.66 -6.28  
6 5344.729 -0.329 K, HI 86 597.55 -4.09 G74 1.88 -6.24  
6 5386.895 -0.305 K, HI 86 743.96 -4.09 G74 1.72 -6.29  
6 5425.880 +0.241 K, HI 87 124.60 -4.09 G74 4.20 -6.39  
5 6024.178 +0.137 K, HI 87 124.60 -4.40 G74 1.37 -6.20  
5 6034.039 -0.209 K, HI 86 597.55 -4.40 G74 2.15 -6.15  
5 6043.084 +0.384 K, HI 87 124.60 -4.40 G74 4.09 -6.41  
5 6034.039 -0.209 K, HI 86 597.55 -4.40 G74 2.15    
S II    $\log N$(S II)/ $N_{\rm tot}$ = -5.12 $\pm$ 0.03    
44 4153.068 +0.617 NIST 128 233.20 - - 8.25 -5.09  
44 4162.665 +0.777 NIST 128 599.16 - - 9.53 -5.13  
1 5027.203 -0.705 NIST 105 599.06 - - 3.05 -5.08  
1 5142.322 -0.822 NIST 106 044.24 - - 1.92 -5.13  
39 5212.620 +0.318 NIST 121 530.02 - - 3.64 -5.17  
6 5453.855 +0.482 NIST 110 268.60 - - 11.70 -5.10  
Ca I    $\log N$(Ca I)/ $N_{\rm tot}$ = -5.26    
2 4226.728 +0.244 NIST 0.00 -5.74 G74 2.4 -5.26  
Ca II   $\log N$(Ca II)/ $N_{\rm tot}$ = -5.67 $\pm$ 0.25    
4 3158.869 +0.252 K, BWL 25 191.51 -5.07 G74 46.4 -5.90  
4 3179.331 +0.512 K, BWL 25 414.40 -5.07 G74 57.4 -5.76  
4 3181.275 -0.448 K, BWL 25 414.40 -5.07 G74 29.7 -5.83  
3 3706.024 -0.447 K, BWL 25 191.51 -5.09 G74   -5.54 Wings of H15, H16
3 3736.902 -0.147 K, BWL 25 414.40 -5.09 G74   -5.60 Red wing of H13
1 3933.664 +0.134 K, BWL 0.00 -5.52 G74   -5.54 Bump on the red wing
1 3968.469 -0.179 K, BWL 0.00 -5.52 G74   -5.54 Blue wing of H $_{\epsilon}$, red component
15 5001.479 -0.517 K, BWL 60 533.53 -4.24 G74   -5.64 Blend with Fe II
15 5019.971 -0.257 K, BWL 60 611.28 -4.24 G74   -5.64 Blend with Fe II
15 5021.138 -1.217 K, BWL 60 611.28 -4.24 G74   -5.54: Weak
14 5285.266 -1.153 K, BWL 60 533.02 -4.30 G74   -5.54: Weak
14 5307.224 -0.853 K, BWL 60 611.28 -4.30 G74   - Blend with an unknown component
13 8201.720 +0.315 K, BWL 60 533.02 -4.62 G74   - Telluric line
13 8248.796 +0.572 NIST 60 611.28 -4.62 G74   -6.40 At the Paschen limit
13 8254.721 -0.388 NIST 60 611.28 -4.62 G74   -5.8?? Weak, at the Paschen limit
2 8498.023 -1.312 K, BWL 13 650.19 -5.55 G74   -5.54 Shifted by +0.2 Å, blue wing of P15
2 8542.091 -0.362 K, BWL 13 710.88 -5.55 G74     No observations
2 8662.141 -0.623 K, BWL 13 650.19 -5.55 G74   -5.20 Shifted by +0.2 Å, blue wing of P13
12 9854.759 -0.228 K, BWL 60 533.02 -4.66 G74   $\le$-5.54 Bad spectrum, low S/N
12 9931.374 +0.072 K, BWL 60 611.28 -4.66 G74   $\le$-5.54 Bad spectrum, low S/N
a "K'' before another $\log~gf$ source means that the $\log~gf$ is from Kurucz files available at http://kurucz.harvard.edu/linelists/gf100
(BBCB) Berry et al. (1971); (BIE) Biémont (1977); (BWL) Black et al. (1972); (CNO) Wiese et al. (1996); (HI) Hibbert (1988); (KP) Kurucz & Peytremann (1975); (LA) Lanz & Artru (1985); (NBS) Wiese et al. (1966); (NIST) http://physics.nist.gov/cgi-bin/AtData/lines-form; (SG) Schulz-Gulde (1969).
b (BCS1) Barnard et al. (1974); (BCS2) Barnard et al. (1975); (DS90) Dimitrijevic & Sahal-Bréchot (1990); (G74) Griem (1974); (LDA) Lanz et al. (1988); (SM69) Shamey (1969).


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