BlackbodySource¶
- class sbpy.spectroscopy.sources.BlackbodySource(T=None)[source]¶
Bases:
sbpy.spectroscopy.sources.SpectralSource
Blackbody sphere.
Spectral flux densities are calculated from
pi * B(T)
, whereB
is the Planck function.- Parameters
- T
Quantity
, required Temperature in Kelvin.
- T
Attributes Summary
Attributes Documentation
- T¶