redback.transient_models.magnetar_driven_ejecta_models.general_mergernova
- redback.transient_models.magnetar_driven_ejecta_models.general_mergernova(time, redshift, mej, beta, ejecta_radius, kappa, n_ism, l0, tau_sd, nn, thermalisation_efficiency, **kwargs)[source]
- Parameters:
time – time in observer frame in days
redshift – redshift
mej – ejecta mass in solar units
beta – initial ejecta velocity
ejecta_radius – initial ejecta radius
kappa – opacity
n_ism – ism number density
l0 – initial magnetar X-ray luminosity
tau_sd – magnetar spin down damping timescale
nn – braking index
thermalisation_efficiency – magnetar thermalisation efficiency
kwargs – Additional parameters
pair_cascade_switch – whether to account for pair cascade losses, default is True
albedo (ejecta) – ejecta albedo; default is 0.5
pair_cascade_fraction – fraction of magnetar luminosity lost to pair cascades; default is 0.05
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’