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Line Identification of Atomic and Ionic Spectra of Holmium in the Near-UV. Part I. Spectrum of Ho I

  • Authors: N. Al-Labady, B. Özdalgiç, A. Er, F. Güzelçimen, I. K. Öztürk, S. Kröger, A. Kruzins, M. Tamanis, R. Ferber, and Gö. Başar

2017 The Astrophysical Journal Supplement Series 228 16.

  • Provider: AAS Journals

Caption: Figure 5.

Three lines between 25,037 and 25,040 cm−1. Besides two classified and simulated lines on the left side, an example of a line with a good S/N and wide hyperfine structure is shown; it cannot be classified on the basis of all known Ho energy levels and has not been found in the extant literature.

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