uvex_transients.models.spectra.thermal#
Blackbody spectral shape.
A BlackbodySpectrum is shaped entirely by a single sampled
temperature – unlike a power law, which is scale-free and needs an
arbitrary reference frequency to anchor it, a blackbody’s shape has no free
normalization choice: the Planck function, normalized by the
Stefan-Boltzmann law, already integrates to exactly 1 over all frequencies
for any temperature.
Classes
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Blackbody spectral shape, shaped entirely by a sampled |