BlackBody

Several blackbody calculations based on temperature and, optionally, wavelength

BlackBody accepts temperature as input and returns total radiance and peak radiance. If wavelengths are also input, spectral radiance and number of photons are also included in the output. If a wavelength range is input, then the total radiance and number of photons within that range are calculated. Output is in a structure, or nicely printed if no output variables are defined by the calling function.