redback.transient_models.afterglow_models.afterglow_models_sed

redback.transient_models.afterglow_models.afterglow_models_sed(time, **kwargs)[source]

A base class for afterglowpy models for bandpass magnitudes/flux/spectra/sncosmo source.

Parameters:

  • time – time in days in observer frame

  • kwargs – Additional keyword arguments, must be all parameters required by the base model and the following:

  • base_model – A string to indicate the type of jet model to use.

  • spread – whether jet can spread, defaults to False

  • latres – latitudinal resolution for structured jets, defaults to 2

  • tres – time resolution of shock evolution, defaults to 100

  • spectype – whether to have inverse compton, defaults to 0, i.e., no inverse compton. Change to 1 for including inverse compton emission.

  • bands – Required if output_format is ‘magnitude’ or ‘flux’.

  • output_format – ‘magnitude’, ‘spectra’, ‘flux’, ‘sncosmo_source’

  • lambda_array – Optional argument to set your desired wavelength array (in Angstroms) to evaluate the SED on.

Returns:

set by output format - ‘magnitude’, ‘spectra’, ‘flux’, ‘sncosmo_source’