redback.transient_models.shock_powered_models.shock_cooling
- redback.transient_models.shock_powered_models.shock_cooling(time, redshift, log10_mass, log10_radius, log10_energy, **kwargs)[source]
- Parameters:
time – time in observer frame in days
redshift – redshift
log10_mass – log10 mass of extended material in solar masses
log10_radius – log10 radius of extended material in cm
log10_energy – log10 energy of extended material in ergs
kwargs – extra parameters to change physics and other settings
frequency – frequency to calculate model on - Must be same length as time array or a single number)
nn – density power law slope
delta – inner density power law slope
frequency – Required if output_format is ‘flux_density’. frequency to calculate - Must be same length as time array or a single number).
bands – Required if output_format is ‘magnitude’ or ‘flux’.
output_format – ‘flux_density’, ‘magnitude’, ‘spectra’, ‘flux’, ‘sncosmo_source’
lambda_array – Optional argument to set your desired wavelength array (in Angstroms) to evaluate the SED on.
cosmology – Cosmology to use for luminosity distance calculation. Defaults to Planck18. Must be a astropy.cosmology object.
- Returns:
set by output format - ‘flux_density’, ‘magnitude’, ‘spectra’, ‘flux’, ‘sncosmo_source’