Table A.3: Abundances of elements with Z $\ge $ 31.
Mult $\lambda$(Å) $\log~gf$ Ref.a $\chi_{{\rm low}}$(cm-1) $\chi_{{\rm up}}$(cm-1) W(mÅ) $\log N$/ $N_{\rm tot}$ Notes
Ga II   $\log N$(Ga II)/ $N_{\rm tot}$ = -5.43 $\pm$ 0.04    
- 4251.149 +0.35 RS94 113 815.92 137 332.35   -5.20  
- 4254.075 -0.23 RS94 113 842.19 137 342.44   -5.20  
- 4255.722 +0.634 NKW, RS94 113 842.19 137 333.33   -5.45 Bad fit, missing components
- 4255.937 -0.32 NKW, RS94 113 842.19 137 332.35   -5.45: Blend with (wrong?) Mn II
- 4262.014 +0.98 RS94 113 883.19 137 339.64   -5.45 Blend with Cr II+Cr II
- 5338.240 +0.43 RS94 118 430.20 137 157.48   -5.65: Bad fit
- 5360.402 +0.42 RS94 118 518.47 137 168.47   -5.45  
- 5363.585 +0.06 NKW 118 518.47 137 157.48   -5.45 Blend with (wrong?) Cr II
- 5416.318 +0.64 RS94 118 727.89 137 185.30   -5.25  
- 5421.275 -0.05 NKW 118 727.89 137 168.47   -5.45  
- 6334.069 +1.00 RS94 102 944.55 118 727.89   -5.65  
- 6419.239 +0.57 RS94 102 944.55 118 518.47   -5.55 Blend with (wrong?) Cr II
- 6455.923 -0.08 RS94 102 944.55 118 430.02   -5.45 Blend with O I
guessed $\log~gf$s for Ga II    
- 4261.478 -1.10 GUESS 113 883.19 137 342.44      
- 4263.136 -0.50 GUESS 113 883.19 137 333.33      
- 5219.658 +0.35 GUESS 120 550.27 139 703.28      
- 7198.450 +0.25 GUESS 106 662.21 120 550.27      
- 7792.260 +0.00 GUESS 107 720.56 120 550.27      
Br II   $\log N$(Br II)/ $N_{\rm tot}$ = -7.12 $\pm$ 0.04    
- 4704.850 +0.408 NIST 93 921.34 115 176.00 1.09 -7.16  
- 4785.500 +0.208 NIST 93 921.54 114 818.00 0.85 -7.07  
Sr II   $\log N$(Sr II)/ $N_{\rm tot}$ = -8.41    
1 4077.709 +0.151 NIST 0.00 24 516.65 26.66 -8.41  
Y II   $\log N$(Y II)/ $N_{\rm tot}$ = -6.66 $\pm$ 0.20    
10 3195.616 -0.420 K, HL 840.21 32 124.04 28.64 -6.35  
10 3200.272 -0.430 K, HL 1045.08 32 283.40 26.37 -6.45  
10 3203.322 -0.370 K, HL 840.21 32 048.78 27.86 -6.44  
10 3216.682 -0.020 K, HL 1045.08 32 124.04 35.67 -6.35  
10 3242.280 +0.210 K, HL 1449.81 32 283.40 40.16 -6.32  
18 3327.878 +0.130 K, CC 3296.18 33 336.72 32.32 -6.51  
3 3496.081 -0.720 K, HL 0.00 28 595.27 20.64 -6.48  
9 3549.005 -0.280 K, HL 1045.08 29 213.95 27.34 -6.48  
9 3584.514 -0.410 K, HL 840.21 28 730.01 24.78 -6.49  
9 3600.741 +0.280 K, HL 1044.81 29 213.95 42.41 -6.24  
9 3601.919 -0.180 K, HL 840.21 28 595.27 32.75 -6.30  
9 3611.044 +0.110 K, HL 1045.08 28 730.07 33.79 -6.52  
2 3633.122 -0.100 K, HL 1045.08 27 516.69 30.44 -6.54  
7 3818.341 -0.980 K, HL 1045.08 27 227.04 23.35 -6.90  
16 3930.660 -1.610 K, HL 3296.18 28 730.01 8.63 -6.76  
6 3950.352 -0.490 K, HL 840.21 26 147.25 39.01 -6.84  
16 3951.593 -1.980 K, HL 3296.18 28 595.27 3.22 -6.88  
6 3982.594 -0.490 K, HL 1045.08 26 147.25 36.23 -6.94  
5 4199.277 -2.150 K, HL 840.21 24 647.13 3.55 -6.82  
1 4204.695 -1.760 K, HL 0.00 23 776.24 7.89 -6.87  
5 4235.729 -1.500 K, HL 1045.08 24 647.13 10.66 -6.91  
5 4309.631 -0.750 K, HL 1449.81 24 647.13 30.09 -6.89  
5 4358.728 -1.329 K, HL 840.21 23 776.24 14.58 -6.91  
22 4883.684 +0.070 K, HL 8743.32 29 213.94 46.51 -6.64  
22 4900.120 -0.090 K, HL 8328.04 28 730.01 42.70 -6.66  
20 4982.129 -1.290 K, HL 8328.04 28 394.18 7.22 -6.88  
20 5087.416 -0.170 K, HL 8743.32 28 394.18 38.33 -6.72  
20 5119.112 -1.360 K, HL 8003.12 27 532.32 7.41 -6.82  
20 5200.406 -0.570 K, HL 8003.12 27 227.04 25.20 -6.83  
20 5205.724 -0.342 K, HL 8328.04 27 532.32 35.39 -6.68  
27 5473.388 -1.020 K, HL 14 081.26 32 283.40 7.68 -6.76  
27 5480.732 -0.990 K, HL 13 833.38 32 124.04 7.38 -6.82  
27 5497.408 -0.580 K, HL 14 098.07 32 283.40 18.31 -6.68  
27 5546.009 -1.100 K, HL 14 098.07 32 124.04 7.44 -6.69  
38 5662.925 +0.160 K, CC 15 682.90 33 336.72 40.07 -6.51  
34 5728.890 -1.120 K, HL 14 832.85 32 283.40 5.61 -6.76  
32 7881.881 -0.572 K, HL 14 832.85 27 516.69 11.95 -6.82  
Zr II   $\log N$(Zr II)/ $N_{\rm tot}$ = -8.67 $\pm$ 0.17    
3 3279.266 -0.230 K, CC' 736.44 31 249.28 2.47 -8.35  
1 3391.982 +0.463 K, CC' 1322.91 30 795.74 5.15 -8.63  
46 3479.383 +0.170 K, BG 5752.92 34 485.42 1.00 -8.83  
10 3496.192 +0.189 K, CC 314.67 28 909.04 2.60 -8.78  
41 4149.217 -0.030 K, CC 6467.61 30 561.75 2.34 -8.78  
Rh II   $\log N$(Rh II)/ $N_{\rm tot}$ = -8.50:    
1 3162.284 +0.000 K, GUESS 28 834.60 60 448.40      
5 3187.875 +0.000 K, GUESS 27 801.40 59 161.50      
1 3207.285 +0.000 K, GUESS 25 376.90 56 547.30      
2 3233.314 +0.000 K, GUESS 27 439.40 58 358.50      
6 3267.480 +0.000 K, GUESS 31 730.50 62 326.10      
5 3307.348 +0.000 K, GUESS 28 131.40 58 358.50      
4 3477.823? +0.000 K, GUESS 27 801.40 56 547.30      
Pd I   $\log N$(Pd I)/ $N_{\rm tot}$ = -6.41 $\pm$ 0.30    
3 3242.700 -0.070 K, BG 6564.11 37 393.71 3.63 -5.96  
2 3404.579 +0.320 K, BG 6564.11 35 927.89 2.67 -6.47  
9 3553.080 +0.540 K, CB 11 721.77 39 858.33 0.82 -6.89  
2 3609.547 +0.050 K, BG 7754.40 35 451.40 1.39 -6.40  
1 3634.690 +0.090 K, CB 6564.11 34 068.93 2.02 -6.33  
Xe II   $\log N$(Xe II)/ $N_{\rm tot}$ = -5.96 $\pm$ 0.20    
- 4603.01 0.018 WM80 95 064.00 116 783.00 3.62 -6.32  
- 4844.33 0.491 WM80 93 068.00 113 705.00 11.33 -6.04  
- 5292.22 0.351 WM80 93 068.00 111 959.00 10.80 -5.81  
- 5372.39 -0.211 WM80 95 064.00 113 673.00 3.12 -5.96  
- 5419.15 0.215 WM80 95 064.00 113 512.00 7.75 -5.80  
- 5719.60 -0.746 WM80 96 033.00 113 512.00 1.79 -5.58  
- 5976.46 -0.222 WM80 95 054.00 111 782.00 1.60 -6.12  
- 6051.15 -0.252 WM80 95 438.00 111 959.00 1.46 -6.12  
- 6097.59 -0.237 WM80 95 397.00 111 792.00 1.94 -5.99  
- 6990.88 +0.200 WM80 99 405.00 113 705.00 2.52 -5.86 $\lambda_{{\rm obs}}$ = 6990.82 Å
Other identified weak Xe II lines    
- 5260.44 -0.437 WM80 104 250.00 123 255.00      
- 5261.95 +0.150 WM80 112 925.00 131 924.00      
- 5438.96 -0.183 WM80 102 799.00 121 180.00      
- 5472.61 -0.449 WM80 95 437.00 113 705.00     Blend Cr II
- 5531.07 -0.616 WM80 95 437.00 113 512.00      
- 6036.20 -0.609 WM80 95 397.00 111 959.00      
identified Xe II lines with no available $\log~gf$    
- 4448.13 0.00 GUESS 123 112.54 145 587.61      
- 4921.48 0.00 GUESS 102 799.07 123 112.54      
- 5339.33 0.00 GUESS 93 068.44 111 792.17      
- 5368.07 0.00 GUESS 105 947.55 124 571.09      
- 5525.53 0.00 GUESS 124 289.45 142 382.13      
- 5667.56 0.00 GUESS 96 033.48 113 679.89      
Ba II   $\log N$(Ba II)/ $N_{\rm tot}$ = -9.27    
- 4554.029 +0.163 K, NBS 0.00 21 952.42   -9.27  
- 4934.076 -0.150 K, NBS 0.00 20 261.56 1.041 -9.35  
Pr III   $\log N$(Pr III)/ $N_{\rm tot}$ = -9.62    
- 5299.969 -0.530 DREAM 2893.14 21 755.84   -9.62  
Nd III   $\log N$(Nd III)/ $N_{\rm tot}$ = -9.57 $\pm$ 0.08    
- 5127.044 -1.080 DREAM 2388.00 21 887.00 1.08 -9.50  
- 5203.924 -1.190 DREAM 0.00 19 211.00 0.82 -9.65  
Yb II   $\log N$(Yb II)/ $N_{\rm tot}$ = -8.10 $\pm$ 0.19    
- 3478.834 +0.460 DREAM 30 224.33 58 961.37 3.457 -7.82  
- 4180.810 -0.290 DREAM 30 392.23 54 304.30 1.064 -8.33  
- 5335.159 -0.260 DREAM 30 562.79 49 301.16 1.865 -8.08  
- 5352.954 -0.340 DREAM 30 224.33 48 900.41 1.280 -8.19  
Yb III   $\log N$(Yb III)/ $N_{\rm tot}$ = -7.31 $\pm$ 0.01    
- 3325.514 -1.35 DREAM 42 425.00 72 487.00 3.24 -7.31  
- 3384.013 -0.58 DREAM 53 365.00 82 907.00 3.63 -7.32  
Pt II   $\log N$(Pt II)/ $N_{\rm tot}$ = -7.63    
- 4514.124 -1.48 DSJ 29 261.97 51 408.37   -7.63  
Au II   $\log N$(Au II)/ $N_{\rm tot}$ = -7.51 $\pm$ 0.06    
- 4016.672 -1.88 RW 48 510.89 73 403.84 1.06 -7.58  
- 4052.790 -1.69 RW 48 510.89 73 178.29 2.09 -7.45  
Hg I   $\log N$(Hg I)/ $N_{\rm tot}$ = -6.19 $\pm$ 0.18    
- 4046.599 -0.818 BLD 37 645.08 62 350.46 0.89 -6.37  
- 5460.731 -0.185 BLD 44 042.98 62 350.46 3.05 -6.01  
Hg II   $\log N$(Hg II)/ $N_{\rm tot}$ = -6.53 $\pm$ 0.23    
- 3983.890 -1.520 PS,SR 35 514.00 60 608.00   -6.30  
- 6149.470 +0.150 SR 95 714.41 111 971.46 1.95 -6.58  
a "K'' before another $\log~gf$ source means that the $\log~gf$ is from Kurucz files available at http://kurucz.harvard.edu/linelists/gf100
(BLD) Benck et al. (1989); (BG) Biémont et al. (1981); (CB) Corliss & Bozman (1962); (CC) Cowley & Corliss (1983); (CC') Cowley & Corliss (1983), out the fitting range; (DJS) Dworetsky et al. (1984); (DREAM) Biémont et al. (1999), http://www.umh.ac.be/astro/dream.shtml; (GUESS) guessed values; (HL) Hannaford et al. (1982); (NBS) Miles & Wiese (1969); (NIST) http://physics.nist.gov/cgi-bin/AtData/lines-form; (NKW) Nielsen et al. (2000); (PS) Proffitt et al. (1999); (SR) Sansonetti & Reader (2001); (RS94) Ryabchikova & Smirnov (1994); (RW) Rosberg & Wyart (1997); (WM80) Wiese & Martin (1980).


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