Public module which computes the thermal spectra from a given set of kilonova parameters. Wrapper to the FORTRAN library for the SAEE model.


compute_planck_function(lambda_cm, temperature)

Planck function of wavelength.

create_saee_seds(KNE_parameters[, min_wave, ...])

Function which prepares the inputs from the python code to the fortran library to compute the bolometric luminosity evolution for a kilonova given the input generating parameters.

create_sed_timeseries(luminosity_array[, ...])

Function to compute a planck distribution normalized to sigma*T**4/pi