Derives Teff, log g and metallicity for 282 M dwarfs via χ² fits of updated PHOENIX models to simultaneous visible+NIR CARMENES spectra, finding visible and combined ranges superior to NIR alone.
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MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.
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The CARMENES search for exoplanets around M dwarfs -- Photospheric parameters of target stars from high-resolution spectroscopy. II. Simultaneous multiwavelength range modeling of activity insensitive lines
Derives Teff, log g and metallicity for 282 M dwarfs via χ² fits of updated PHOENIX models to simultaneous visible+NIR CARMENES spectra, finding visible and combined ranges superior to NIR alone.
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Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.