Synthetic Photometry
Model:
AMES-Dusty 2000
The AMES-Dusty Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation but including dust opacity (fully efficient dust settling). Wavelengths have been converted to air wavelengths.
Model parameters
Teff: - (?)
Logg: - (?)

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λmean:- A
Facility
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Please, select the parameter values that you are interested in
 

References:

 
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