Synthetic Photometry
Model:
Keck LRIS spectra of late-M, L and T dwarfs
These spectra were obtained between 1997 and 1999; they are all flux calibrated and generally span the wavelength range 6000-10,000 A. Spectral types are on the Kirkpatrick et al system as defined in Kirkpatrick et al ApJS, 77, 417 (1991 - for M dwarfs) and Kirkpatrick et al ApJ 519, 802 (1999 - L dwarfs). While not all of these stars are primary spectral standards, they are all bright and should provide an adequate reference sequence.
Model parameters
SpTy:(?)

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 2008