redback.transient_models.supernova_models.basic_magnetar_powered

redback.transient_models.supernova_models.basic_magnetar_powered(time, redshift, p0, bp, mass_ns, theta_pb, **kwargs)[source]
Parameters:

  • time – time in days in observer frame

  • redshift – source redshift

  • p0 – initial spin period

  • bp – polar magnetic field strength in Gauss

  • mass_ns – mass of neutron star in solar masses

  • theta_pb – angle between spin and magnetic field axes

  • kwargs – Must be all the kwargs required by the specific interaction_process, photosphere, sed methods used e.g., for Diffusion and TemperatureFloor: kappa, kappa_gamma, vej (km/s), temperature_floor

  • interaction_process – Default is Diffusion. Can also be None in which case the output is just the raw engine luminosity, or another interaction process.

  • photosphere – Default is TemperatureFloor. kwargs must have vej or relevant parameters if using different photosphere model

  • sed – Default is blackbody.

  • 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’