colour.plotting.plot_blackbody_spectral_radiance#
- colour.plotting.plot_blackbody_spectral_radiance(temperature: float = 3500, cmfs: MultiSpectralDistributions | str | Sequence[MultiSpectralDistributions | str] = 'CIE 1931 2 Degree Standard Observer', blackbody: str = 'VY Canis Major', **kwargs: Any) Tuple[Figure, Axes][source]#
Plot the spectral radiance of a blackbody at the specified temperature.
- Parameters:
temperature (float) – Blackbody temperature.
cmfs (MultiSpectralDistributions | str | Sequence[MultiSpectralDistributions | str]) – Standard observer colour matching functions used for computing the spectrum domain and colours.
cmfscan be of any type or form supported by thecolour.plotting.common.filter_cmfs()definition.blackbody (str) – Blackbody name.
kwargs (Any) – {
colour.plotting.artist(),colour.plotting.plot_single_sd(),colour.plotting.render()}, See the documentation of the previously listed definitions.
- Returns:
Current figure and axes.
- Return type:
Examples
>>> plot_blackbody_spectral_radiance(3500, blackbody="VY Canis Major") ... (<Figure size ... with 2 Axes>, <...Axes...>)