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Table C.3

Remaining unidentified lines in the spectra of LS IV–14°116 and Feige 46.

λobs (Å) EW (mÅ) Comment
3330.784 14.6 Kr III?
3439.421 13.3 Kr III, Rb III?
3457.789 11.3 Sr III?
3492.674 6.2 Kr III, Rb III?
3530.783 7.9 Zn III?
3570.183 4.5 Ne II?
3647.659 4.4
3649.103 4.2
3853.263 7.1
3857.237 4.8
3860.431 8.0
3863.822 7.8
3870.852 6.0 Ni III?
3873.239 3.0
3901.527 5.3
3912.595 4.5 Sr IV?
3915.091 5.3
3931.572 5.2
3931.572 5.2
3935.767 9.5
4013.975 4.1
4037.023 6.5
4050.439 4.8
4058.837 4.4
4059.791 2.6
4088.011 4.7
4148.989 13.0
4181.054 7.5 Kr IV?
4184.853 5.1
4210.418 1.8
4211.177 1.8
4479.618 14.0
4636.534 35.0 Not covered for LS IV–14°116
Broad
4814.473 14.0
4820.085 9.2
4879.165 5.3
4972.468 8.1
5102.885 16.5 Weaker in Feige 46, Sn III?
5106.656 6.6
5114.154 12.9 Very broad
5135.913 13.9 Broad
5167.776 6.2
5207.452 4.1
5208.282 3.5
5210.208 2.8 Stronger in Feige 46
5221.968 9.4 Weaker in Feige 46
5232.749 5.9
5234.305 5.7 Not det. in Feige 46
5241.974 6.2
5562.854 8.3 Zn III?
6756.452 16.3 Not covered for Feige 46

Notes. Estimated equivalent widths are given forLS IV–14°116. The detection limit is about 1.5 mÅ.

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