Line-by-line opacity stellar model atmospheres

By D. Shulyak, V. Tsymbal, T. Ryabchikova, Ch. Stütz, W. Weiss. 2004

266 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/8853a15727f87498c08acfa3644d6ebb8170a2de

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. S. Hekker
2. H. Kjeldsen
3. N. Piskunov
4. R. García
5. J. Valenti
6. J. Christensen-Dalsgaard
7. B. Smalley
8. J. Cleve

In Instrumentation

1. S. Hekker
2. N. Piskunov
3. J. Valenti
4. B. Smalley
5. J. Christensen-Dalsgaard
6. M. Still
7. H. Kjeldsen
8. S. Thompson

Citations in the corpus

• Spectroscopy Made Easy: Evolution (2016, methodology): “For solar-type atmospheres in an ATLAS9 grid, the maximum errors are 1.4% for interpolation along the Teff axis with a grid spacing of 250 K, 0.1% along the log g axis for 0.5 dex spacing, and 0.2% along the [m/H] axis with 0.1 dex spacing.”
• The Kepler characterization of the variability among A- and F-type stars I. General overview (2011, methodology): “The synthetic spectra have been computed with the SynthV programme (Tsymbal 1996) based on atmosphere models computed with LLmodels (Shulyak et al. 2004).”