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Stellar population astrophysics (SPA) with the TNG. Identification of a sulphur line at λ_air = 1063.6 nm in GIANO-B stellar spectra

Ryde, N. (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Hartman, Henrik (author)
Malmö University,Lund University,Lunds universitet,Malmö universitet,Institutionen för materialvetenskap och tillämpad matematik (MTM),Lund Observatory, Department of Astronomy and Theoretical Physics, Lund University, Box 43 221 00 Lund, Sweden,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Oliva, E. (author)
INAF - Osservatorio Astrofisico di Arcetri
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Origlia, L. (author)
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna
Sanna, N. (author)
INAF - Osservatorio Astrofisico di Arcetri
Rainer, M. (author)
INAF - Osservatorio Astrofisico di Arcetri
Thorsbro, B. (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Dalessandro, E. (author)
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna
Bono, G. (author)
INAF-Osservatorio Astronomico di Roma,University of Rome Tor Vergata
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 (creator_code:org_t)
2019-10-23
2019
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 631, s. L3-L5
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Context. In the advent of new infrared, high-resolution spectrometers, accurate and precise atomic data in the infrared is urgently needed. Identifications, wavelengths, strengths, broadening and hyper-fine splitting parameters of stellar lines in the near-IR are in many cases not accurate enough to model observed spectra, and in other cases even non existing. Some stellar features are unidentified. Aims. The aim with this work is to identify a spectral feature at lambda(vac) = 1063.891 nm or lambda(air) = 1063.600 nm seen in spectra of stars of different spectral types, observed with the GIANO-B spectrometer. Methods. Searching for spectral lines to match the unidentified feature in linelists from standard atomic databases was not successful. However, by investigating the original, published laboratory data we were able to identify the feature and solve the problem. To confirm its identification, we model the presumed stellar line in the solar intensity spectrum and find an excellent match. Results. We find that the observed spectral feature is a stellar line originating from the 4s'-4p' transition in S I, and that the reason for its absence in atomic line databases is a neglected air-to-vacuum correction in the original laboratory measurements from 1967 for this line only. From interpolation we determine the laboratory wavelength of the S I line to be lambda(vac) = 1063.8908 nm or lambda(air) = 1063.5993 nm, and the excitation energy of the upper level to be 9.74978 eV.

Subject headings

NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

atomic data
infrared
stars
line
identification
instrumentation
spectrographs
methods
laboratory atomic
techniques
spectroscopic
solar astrophysics
stellar astrophysics
astrophysics
Atomic data
Infrared: Stars
Instrumentation: Spectrographs
Line: Identification
Methods: Laboratory: Atomic
Techniques: Spectroscopic

Publication and Content Type

ref (subject category)
art (subject category)

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