1996
DOI: 10.1086/192333
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Infrared Spectral Atlases of the Sun from NOAO

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Cited by 95 publications
(83 citation statements)
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“…Temperatures as low as ~ 3000 K, however, are found in sunspots. We noticed a large number of unassigned lines in two sunspot atlases (Wallace et al 1996). We suspected that these lines were due to hot water but the available laboratory data were inadequate to confirm this.…”
Section: Sunspots and Laboratory Experimentsmentioning
confidence: 96%
“…Temperatures as low as ~ 3000 K, however, are found in sunspots. We noticed a large number of unassigned lines in two sunspot atlases (Wallace et al 1996). We suspected that these lines were due to hot water but the available laboratory data were inadequate to confirm this.…”
Section: Sunspots and Laboratory Experimentsmentioning
confidence: 96%
“…Spectroscopic orbital solutions for EW Ori determined from re-analyses of the radial velocity observations by Popper et al (1986) and Imbert (2002 recent grid of MARCS model atmospheres (Gustafsson et al 2008), which adopt the solar composition by Grevesse et al (2007). Line information was taken from the Vienna Atomic Line Database (VALD; Kupka et al 1999), but in order to derive abundances relative to the Sun, log(g f ) values have been adjusted in such a way that each measured line in the Wallace et al (1998) solar atlas reproduces the atmospheric abundances by Grevesse et al (2007). Analyses of a FEROS sky spectrum reproduce these adjustments closely.…”
Section: Chemical Abundancesmentioning
confidence: 99%
“…Infrared spectral atlases of the Sun have been published (Wallace et al 1996), which are of value for spectroscopic studies of highly excited states of some molecules.…”
Section: Fundamental Data and Databasesmentioning
confidence: 99%