redback.transient_models.kilonova_models.one_component_nsbh_ejecta_relation
- redback.transient_models.kilonova_models.one_component_nsbh_ejecta_relation(time, redshift, mass_bh, mass_ns, chi_bh, lambda_ns, kappa, **kwargs)[source]
One component NSBH model
- Parameters:
time – observer frame time in days
redshift – redshift
mass_bh – mass of black hole
mass_2 – mass of neutron star
chi_bh – spin of black hole along z axis
lambda_ns – tidal deformability of neutron star
kappa – opacity
kwargs – additional keyword arguments
temperature_floor – floor temperature
ejecta_relation – a class that relates the instrinsic parameters to the kilonova parameters default is OneComponentNSBH
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’