BlackbodySource

class sbpy.spectroscopy.sources.BlackbodySource(T=None)[source] [edit on github]

Bases: SpectralSource

Blackbody sphere.

Spectral flux densities are calculated from pi * B(T), where B is the Planck function.

Parameters:
TQuantity, required

Temperature in Kelvin.

Attributes Summary

T

Attributes Documentation

T