Atomic lines in infrared spectra for ultracool dwarfs

Abstract

We provide a set of atomic lines which are suitable for the description of ultracool dwarf spectra from 10000 to 25000 Å. This atomic linelist was made using both synthetic spectra calculations and existing atlases of infrared spectra of Arcturus and Sunspot umbra. We present plots, which show the comparison of synthetic spectra and observed Arcturus and Sunspot umbral spectra for all atomic lines likely to be observable in high resolution infrared spectra.

21 pages, 2 tables, 129 figures, figures are available only at http://www.astro.livjm.ac.uk/~hraj/spectralatlas/index.html, accepted to A&A

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Cited by in corpus (8)

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• Prospects for population synthesis in the H band: NeMo grids of stellar atmospheres compared to observations
• F, G, K, M Spectral Standards in the Y Band (0.95-1.11 um)
• Infrared Telescope Facility (IRTF) spectral library II: New indices in Y, J, H, and L atmospheric windows