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Synthetic Photometry
Model:
BT-DUSTY
The BT-DUSTY Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation but including dust opacity (fully efficient dust settling) and updated abundances. Wavelengths have been converted to air wavelengths.
Model parameters
Teff: - (?)
Logg: - (?)
Metallicity: - (?)

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