redback.transient_models.shock_powered_models.shocked_cocoon

redback.transient_models.shock_powered_models.shocked_cocoon(time, redshift, mej, vej, eta, tshock, shocked_fraction, cos_theta_cocoon, kappa, **kwargs)[source]
Parameters:

  • time – observer frame time in days

  • redshift – redshift

  • mej – ejecta mass in solar masses

  • vej – ejecta mass in km/s

  • eta – slope for ejecta density profile

  • tshock – shock time in seconds

  • shocked_fraction – fraction of ejecta mass shocked

  • cos_theta_cocoon – cocoon opening angle

  • kappa – opacity

  • kwargs – Extra parameters used by function

  • 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’