Statistics – Computation
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35239058w&link_type=abstract
VizieR On-line Data Catalog: J/A+A/523/A58. Originally published in: 2010A&A...523A..58W
Statistics
Computation
Line Profiles, Spectra: Infrared, Spectroscopy, Stars: Late-Type, Stars: M-Type
Scientific paper
In the pdf atlas (fehatlas.pdf), the identified FeH lines, were assigned with their molecular quantum numbers, which are in detail: lower and upper vibrational state, branch, lower rotational state, lower and upper omega, and the fraction to a possible blend. The latter one is unity if the line is not blended. In the atlas, we plotted the CRIRES spectrum of GJ1002 together with two computed spectra for an M dwarf model with logg=5.0, Teff=3100K and solar composition. One of the synthetic spectra is computed using the original Einstein A values provided by Dulick et al. (2003ApJ...594..651D) (red), the other one is computed with scaled Einstein A values (green). For both computed spectra, the line positions were adjusted. We also provide the spectra of GJ1002 (table2.dat), unscaled computations (table3.dat), and scaled computations (table4.dat). All spectra are normalized to unity.
(5 data files).
Bernath Peter F.
Reiners Ansgar
Seifahrt Andreas
Wende Sebastian
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