6533b825fe1ef96bd1281d82

RESEARCH PRODUCT

Line Identification of Atomic and Ionic Spectra of Holmium in the Near-UV. II. Spectra of Ho ii and Ho iii

N. Al-labadyM. TamanisA. ErF. GüzelçimenI. K. ÖZtürkSelçuk BilirTansel AkGö. BaşarRuvin FerberSophie KrögerB. ÖZdalgiç

subject

PhysicsArgon010504 meteorology & atmospheric sciencesAnalytical chemistrychemistry.chemical_elementIonic bondingAstronomy and Astrophysics01 natural sciencesSpectral lineNeonchemistryExtant taxonSpace and Planetary ScienceIonization0103 physical sciencesAtomic physicsHolmium010303 astronomy & astrophysics0105 earth and related environmental sciencesLine (formation)

description

Fourier Transform spectra of holmium (Ho) in the UV spectral range from 31,530 to 25,000 cm−1 (317 to 400 nm) have been investigated, particularly focusing on the ionic lines. The distinction between the different degrees of ionization (I, II, and III) is based on differences in signal-to-noise ratios from two Ho spectra, which have been measured with different buffer gases, i.e., neon and argon. Based on 106 known Ho ii and 126 known Ho iii energy levels, 97 lines could be classified as transitions of singly ionized Ho and 9 lines could be classified as transitions of doubly ionized Ho. Of the 97 Ho ii lines, 6 have not been listed in the extant literature. Another 215 lines have been assigned to Ho ii, though they could not be classified on the basis of the known energy levels.

https://doi.org/10.3847/1538-4365/228/2/17