The Astrophysical Journal Supplement Series (Jan 2024)

Updated System of S i Levels Using Fourier Transform Infrared Spectroscopy in the Range from 800 to 11,000 cm−1

  • S. Civiš,
  • A. Kramida,
  • E. M. Zanozina,
  • J. Kubišta,
  • P. Kubelík,
  • M. Ferus,
  • V. E. Chernov

DOI
https://doi.org/10.3847/1538-4365/ad6904
Journal volume & issue
Vol. 274, no. 2
p. 32

Abstract

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In this study we report on high-precision laboratory measurements of transition wavenumbers for 172 atomic sulfur lines in the infrared region 800–11,000 cm ^−1 using Fourier transform spectroscopy techniques. Our analysis includes 96 lines that have not been previously measured in the laboratory. We also correct several sulfur energy-level measurements reported in earlier studies. These refined measurements are important for a range of scientific disciplines, such as astrophysics, atmospheric chemistry, and combustion plasma physics. We have used the combined list of all observed lines to derive a refined set of sulfur energy levels. For about half of all nonautoionizing levels, the uncertainties have been reduced by a factor between 2 and 23. From the newly measured nonpenetrating (high- l ) Rydberg levels we have also obtained the first ionization energy of the S atom, IE = 83,559.170(11) cm ^−1 , which is more accurate than the currently recommended value by 2 orders of magnitude. Our analysis has led to a significantly more accurate result than the earlier set of Ritz wavelengths with observed intensities reduced to a common uniform scale and an extended list of recommended transition probabilities.

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