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Submillimeter-wave atmospheric transmission at El Leoncito, Argentina Andes
(Ieee-inst Electrical Electronics Engineers IncPiscatawayEUA, 2005)
Method for calculating the opacity of the atomic lines in stellar atmospheres
(The Astrophysical Journal, 2009)
Method for calculating the opacity of the atomic lines in stellar atmospheres
(The Astrophysical Journal, 2009)
Method for calculating the opacity of the atomic lines in stellar atmospheres
(The Astrophysical Journal, 2009)
Using non-solar-scaled opacities to derive stellar parameters: Toward high-precision parameters and abundances
(EDP Sciences, 2018-12)
In an effort to improve spectroscopic methods of stellar parameters determination, we implemented non-solar-scaled opacities in a simultaneous derivation of fundamental parameters and abundances. We wanted to compare the ...
A new library of theoretical stellar spectra with scaled-solar and α-enhanced mixtures
(Oxford University PressOxford, 2014)
Theoretical stellar libraries have been increasingly used to overcome limitations of empirical
libraries, e.g. by exploring atmospheric parameter spaces not well represented in the
latter. This work presents a new ...
Outer boundary conditions for evolving cool white dwarfs
(EDP Sciences, 2012-10)
Context. White dwarf evolution is essentially a gravothermal cooling process, which, for cool white dwarfs, depends on the treatment of the outer boundary conditions. Aims. We provide detailed outer boundary conditions ...
Atmospheric characterization for sites of interest in millimetric/submillimetric astronomy.
(Universidad de Concepción.Facultad de Ciencias Físicas y Matemáticas, 2023)
Water vapor is the main source of atmospheric opacity for mm/sub-mm astronomy, henee several studies seek to effectively characterize it for site testing puiposes. Reanalysis databases are quickly becoming popular as an ...
Radiative transfer analyses of Titan's tropical atmosphere
(ACADEMIC PRESS INC ELSEVIER SCIENCESAN DIEGO, 2012)
Titan's optical and near-IR spectra result primarily from the scattering of sunlight by haze and its absorption by methane. With a column abundance of 92 km amagat (11 times that of Earth), Titan's atmosphere is optically ...