redback.transient_models.kilonova_models.mosfit_rprocess

redback.transient_models.kilonova_models.mosfit_rprocess(time, redshift, mej, vej, kappa, kappa_gamma, temperature_floor, **kwargs)[source]

A single component kilonova model that should be exactly the same as mosfit’s r-process model. Effectively the only difference to the redback one_component model is the inclusion of gamma-ray opacity in diffusion.

Parameters:

  • time – observer frame time in days

  • redshift – redshift

  • mej – ejecta mass in solar masses of first component

  • vej – minimum initial velocity of first component

  • kappa – gray opacity of first component

  • temperature_floor – floor temperature of first component

  • kappa_gamma – gamma-ray opacity

  • kwargs – Additional keyword arguments

  • 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.

  • dense_resolution – resolution of the grid that the model is actually evaluated on, default is 300

  • 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’