redback.transient_models.general_synchrotron_models.thermal_synchrotron_v2_fluxdensity

redback.transient_models.general_synchrotron_models.thermal_synchrotron_v2_fluxdensity(time, redshift, bG_sh, log_Mdot_vwind, n_ism, logepse, logepsb, xi, p, **kwargs)[source]
Parameters:

  • time – time in source frame in days

  • redshift – redshift

  • bG_sh – Proper-velocity of the shock (bG_sh = Gamma_sh*beta_sh)

  • Mdot_vwind (log) – log10 of the mass loss rate over wind velocity ((solar mass / year)/(km / s))

  • n_ism – the circumburst density of the ISM (cm^-3)

  • logepse – log10 epsilon_e; electron thermalisation efficiency

  • logepsb – log10 epsilon_b; magnetic field amplification efficiency

  • xi – fraction of energy carried by power law electrons

  • p – electron power law slope

  • kwargs – extra parameters to change physics/settings

  • frequency – frequency to calculate model on - Must be same length as time array or a single number)

  • mu – mean molecular weight, default is 0.62

  • mu_e – mean molecular weight per electron, default is 1.18

  • ell_dec – Deceleration parameter defined in eq. (1) of MQ24, default is 1.0

  • f – Volume-filling factor defined in eq. (3) of MQ24, default is 3.0/16.0

  • cosmology – Cosmology to use for luminosity distance calculation. Defaults to Planck18. Must be a astropy.cosmology object.

Returns:

flux density in mJy