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Table A.1

Atomic line data for the list MASH and iron abundances according to M1.

Specie λ (Å) χlow (eV) log gf EW (mÅ) logϵFe Clipped

4445.47 0.09 –5.410 40.9 7.470
4574.72 2.28 –2.970 54.9 7.489
4726.14 3.00 –3.250 18.8 7.588
4808.15 3.25 –2.790 26.9 7.600
4994.13 0.91 –3.002 104.2 7.275
5197.94 4.30 –1.540 36.9 7.525
5198.72 2.22 –2.113 97.2 7.396
5216.27 1.61 –2.082 117.7 7.156
5217.40 3.21 –1.116 111.3 7.282
5236.20 4.19 –1.497 32.4 7.298
5247.05 0.09 –4.975 66.5 7.530
5250.21 0.12 –4.918 64.6 7.462
5285.13 4.43 –1.540 27.9 7.449
5295.31 4.42 –1.590 29.5 7.518
5379.58 3.69 –1.514 61.5 7.505
5397.62 3.63 –2.528 28.0 7.702
5491.83 4.19 –2.188 13.4 7.445
5517.06 4.21 –2.370 17.5 7.791
5522.45 4.21 –1.450 42.9 7.463
5607.66 4.15 –3.437 14.6 8.699
5638.26 4.22 –0.770 76.1 7.394
5662.52 4.18 –0.573 92.8 7.402
5679.02 4.65 –0.820 59.0 7.501
5778.45 2.59 –3.430 22.1 7.409
5807.78 3.29 –3.410 8.5 7.563
5852.22 4.55 –1.230 39.3 7.470
5855.08 4.61 –1.478 23.8 7.441
5858.78 4.22 –2.160 12.2 7.383
5916.25 2.45 –2.914 54.1 7.471
5930.18 4.65 –0.230 86.8 7.335
6065.48 2.61 –1.470 116.7 7.285
6082.71 2.22 –3.571 33.7 7.456
6105.13 4.55 –2.532 12.8 8.084
6151.62 2.18 –3.312 50.0 7.494
6200.31 2.61 –2.405 73.4 7.497
6213.43 2.22 –2.481 82.6 7.386
6229.23 2.85 –2.805 37.6 7.379
6252.56 2.40 –1.727 119.8 7.437
6421.35 2.28 –2.020 103.7 7.326
6481.88 2.28 –2.985 62.4 7.497
6518.37 2.83 –2.373 59.0 7.361
6608.03 2.28 –3.930 17.6 7.428

4491.40 2.84 –2.710 77.8 7.468
4508.29 2.84 –2.440 84.8 7.313
4582.83 2.83 –3.180 57.0 7.455
4620.52 2.82 –3.210 50.3 7.304
5197.58 3.22 –2.220 81.4 7.315
5264.81 3.22 –3.130 44.3 7.434
5284.11 2.88 –3.195 59.9 7.525
5414.07 3.21 –3.580 25.6 7.414
5425.26 3.20 –3.220 41.5 7.429
5991.38 3.15 –3.647 29.5 7.506
6239.95 3.89 –3.573 13.8 7.635
6247.56 3.89 –2.435 52.1 7.512
6369.46 2.89 –4.110 18.6 7.407
6432.68 2.89 –3.570 41.3 7.442
6456.38 3.90 –2.185 61.5 7.456

Notes. The data presented here corresponds to all the lines with EW ≤ 120 mÅ on the solar spectrum of Ganymede. Some of these lines were excluded as a result of a σ-clipping to produce the final abundances for the Sun. These are indicated with an symbol in the last column of the table.

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