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CRIRES-POP : a library of high resolution spectra in the near-infrared II. Data reduction and the spectrum of the K giant 10 Leonis

Nicholls, Christine P (författare)
Institute for Astrophysics, University of Vienna, Türkenschanzstrasse 17, Vienna, 1180, Austria,University of Innsbruck
Lebzelter, T (författare)
Institute for Astrophysics, University of Vienna, Türkenschanzstrasse 17, Vienna, 1180, Austria
Smette, A (författare)
European Southern Observatory, Casilla 19001, Alonso de Cordova, Vitacura, Santiago, 3107, Chile
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Wolff, B (författare)
European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching bei München, 85748, Germany
Hartman, Henrik (författare)
Malmö University,Lund University,Lunds universitet,Malmö högskola,Institutionen för materialvetenskap och tillämpad matematik (MTM),Lund Observatory, Lund University, Box 43, Lund, 22100, 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,European Southern Observatory
Käufl, H.-U. (författare)
European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching bei München, 85748, Germany
Przybilla, N. (författare)
Institut für Astro-und Teilchenphysik, Universität Innsbruck, Technikerstr. 25/8, Innsbruck, 6020, Austria
Ramsay, S. (författare)
European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching bei München, 85748, Germany
Uttenthaler, S. (författare)
Institute for Astrophysics, University of Vienna, Türkenschanzstrasse 17, Vienna, 1180, Austria,University of Göttingen
Wahlgren, G. M. (författare)
CSRA/STScI, 3700 San Martin Drive, Baltimore, 21218, MD, United States,Space Telescope Science Institute
Bagnulo, G (författare)
Armagh Observatory, College Hill, Armagh, BT619DG, United Kingdom
Hussain, G (författare)
European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching bei München, 85748, Germany; Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, UPS-OMP, Toulouse, 31400, France
Nieva, M.-F. (författare)
Institut für Astro-und Teilchenphysik, Universität Innsbruck, Technikerstr. 25/8, Innsbruck, 6020, Austria
Seemann, U (författare)
Institut für Astrophysik, Georg-August Universität Göttingen, Friedrich-Hund-Platz 1, Göttingen, 37077, Germany
Seifahrt, A. (författare)
Department of Astronomy and Astrophysics, University of Chicago, 5640 S Ellis Avenue, Chicago, 60637, IL, United States
Bagnulo, S. (författare)
Armagh Observatory
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 (creator_code:org_t)
2017-02-03
2017
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 598
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Context. High resolution stellar spectral atlases are valuable resources to astronomy. They are rare in the 1 − 5 μm region for historical reasons, but once available, high resolution atlases in this part of the spectrum will aid the study of a wide range of astrophysical phenomena. Aims. The aim of the CRIRES-POP project is to produce a high resolution near-infrared spectral library of stars across the H-R diagram. The aim of this paper is to present the fully reduced spectrum of the K giant 10 Leo that will form the basis of the first atlas within the CRIRES-POP library, to provide a full description of the data reduction processes involved, and to provide an update on the CRIRES-POP project. Methods. All CRIRES-POP targets were observed with almost 200 different observational settings of CRIRES on the ESO Very Large Telescope, resulting in a basically complete coverage of its spectral range as accessible from the ground. We reduced the spectra of 10 Leo with the CRIRES pipeline, corrected the wavelength solution and removed telluric absorption with Molecfit, then resampled the spectra to a common wavelength scale, shifted them to rest wavelengths, flux normalised, and median combined them into one final data product. Results. We present the fully reduced, high resolution, near-infrared spectrum of 10 Leo. This is also the first complete spectrum from the CRIRES instrument. The spectrum is available online. Conclusions. The first CRIRES-POP spectrum has exceeded our quality expectations and will form the centre of a state-of-the-art stellar atlas. This first CRIRES-POP atlas will soon be available, and further atlases will follow. All CRIRES-POP data products will be freely and publicly available online.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

Atlases - Stars
Stars: atmospheres
Stars: late-type
Infrared: stars
Techniques: spectroscopic
Atlases
Atmospheric effects
Infrared: stars
Stars: atmospheres
Stars: late-type
Techniques: spectroscopic

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