redback.transient_models.tde_models.cooling_envelope

redback.transient_models.tde_models.cooling_envelope(time, redshift, mbh_6, stellar_mass, eta, alpha, beta, **kwargs)[source]

This model is only valid for time after circulation. Use the gaussianrise_metzgertde model for the full lightcurve

Parameters:

  • time – time in observer frame in days

  • redshift – redshift

  • mbh_6 – mass of supermassive black hole in units of 10^6 solar mass

  • stellar_mass – stellar mass in units of solar masses

  • eta – SMBH feedback efficiency (typical range: etamin - 0.1)

  • alpha – disk viscosity

  • beta – TDE penetration factor (typical range: 1 - beta_max)

  • kwargs – Additional parameters

  • 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’