redback.transient_models.supernova_models.type_1c

redback.transient_models.supernova_models.type_1c(time, redshift, f_nickel, mej, pp, **kwargs)[source]

A nickel powered explosion with synchrotron and blackbody SED’s for SNe 1C.

Parameters:

  • time – time in days in observer frame

  • redshift – source redshift

  • f_nickel – fraction of nickel mass

  • mej – ejecta mass in solar masses

  • pp – power law index for synchrotron

  • kwargs – kappa, kappa_gamma, vej (km/s), temperature_floor (K), nu_max (default is 1e9 Hz) source_radius (default is 1e13), f0: synchrotron normalisation (default is 1e-26).

  • 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’