Spectra of a Holmium in the near-UV. I. Ho I. Virtual Observatory Resource

Authors
  1. Al-Labady N.
  2. Ozdalgic B.
  3. Er A.
  4. Guzelcimen F.
  5. Ozturk I.K.
  6. Kroger S.,Kruzins A.
  7. Tamanis M.
  8. Ferber R.
  9. Basar G.
  10. Published by
    CDS
Abstract

The Fourier Transform spectra of a Holmium hollow cathode discharge lamp have been investigated in the UV spectral range from 25000 up to 31530cm^-1^ (317 to 400nm). Two Ho spectra have been measured with neon and argon as buffer gases. Based on the intensity ratios from these two spectra, a distinction was made between atomic and ionic lines (ionic lines are discussed in an accompanying paper). Using the known Ho I energy levels, 71 lines could be classified as transitions of atomic Ho, 34 of which have not been published previously. Another 32 lines, which could not be classified, are listed in the literature and assigned as atomic Ho. An additional 370 spectral lines have been assigned to atomic Ho based on the signal-to-noise ratio in the two spectra measured under different discharge conditions, namely with buffer gases argon and neon, respectively. These 370 lines have not been previously listed in the literature.

Keywords
  1. Atomic physics
  2. Spectroscopy
  3. Ultraviolet astronomy
Bibliographic source Bibcode
2017ApJS..228...16A
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/228/16
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJS/228/16
Document Object Identifer DOI
doi:10.26093/cds/vizier.22280016

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History

2017-04-28T09:41:31Z
Resource record created
2017-04-28T09:41:31Z
Created
2017-06-08T12:28:15Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr