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: - (?)

Show:

Filters
Show only filters with:
λmean:- A
Facility
Instrument
(You can select 50 filters at most, the rest will be ignored)
Please, select the parameter values that you are interested in
 

References:

 
© CAB 2019