redback.transient_models.supernova_models.shocked_cocoon_csm_and_arnett

redback.transient_models.supernova_models.shocked_cocoon_csm_and_arnett(time, redshift, E_eng, t_eng, theta_0, M_csm, R_csm, kappa, f_nickel, mej, vej, **kwargs)[source]
Parameters:

  • time – time in observer frame in days

  • redshift – redshift

  • E_eng – jet energy (erg)

  • t_eng – jet activity timescale (s)

  • theta_0 – jet opening angle (radians)

  • M_csm – CSM mass (solar masses)

  • R_csm – CSM outer radius (cm)

  • kappa – opacity (cm^2/g)

  • f_nickel – Fraction of ejecta made of 56Ni

  • mej – ejecta mass (solar masses)

  • vej – ejecta velocity (km/s)

  • kwargs – Extra parameters used by model e.g., kappa_gamma, temperature_floor, and any kwarg to change any other input physics/parameters from default.

  • 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’