Source code for hierarc.Likelihood.LensLikelihood.td_mag_likelihood

import numpy as np
from lenstronomy.Util import constants as const
from lenstronomy.Util.data_util import magnitude2cps


[docs] class TDMagLikelihood(object): """Likelihood of time delays and magnification likelihood. This likelihood uses linear flux units and linear lensing magnifications. """ def __init__( self, time_delay_measured, cov_td_measured, amp_measured, cov_amp_measured, fermat_diff, magnification_model, cov_model, magnitude_zero_point=20, ): """ :param time_delay_measured: array, relative time delays (relative to the first image) [days] :param cov_td_measured: 2d array, error covariance matrix of time delay measurement [days^2] :param amp_measured: array, amplitudes of measured fluxes of image positions :param cov_amp_measured: 2d array, error covariance matrix of the measured amplitudes :param fermat_diff: mean Fermat potential differences (relative to the first image) in arcsec^2 :param magnification_model: mean magnification of the model prediction :param cov_model: 2d array (length relative time delays + image amplitudes); model fermat potential differences and lensing magnification covariances :param magnitude_zero_point: magnitude zero point for which the image amplitudes and covariance matrix are defined """ self._data_vector = np.append(time_delay_measured, amp_measured) self._cov_td_measured = np.array(cov_td_measured) self._cov_amp_measured = np.array(cov_amp_measured) # check sizes of covariances matches n_tot = len(self._data_vector) self._n_td = len(time_delay_measured) self._n_amp = len(amp_measured) assert self._n_td == len(cov_td_measured) assert self._n_amp == len(cov_amp_measured) assert n_tot == len(cov_model) # merge data covariance matrices from time delay and image amplitudes self._cov_data = np.zeros((n_tot, n_tot)) self._cov_data[: self._n_td, : self._n_td] = self._cov_td_measured self._cov_data[self._n_td :, self._n_td :] = self._cov_amp_measured # self._fermat_diff = fermat_diff # in units arcsec^2 self._fermat_unit_conversion = ( const.Mpc / const.c / const.day_s * const.arcsec**2 ) # self._mag_model = mag_model self._model_tot = np.append(fermat_diff, magnification_model) self._cov_model = cov_model self.num_data = n_tot self._magnitude_zero_point = magnitude_zero_point
[docs] def log_likelihood(self, ddt, mu_intrinsic): """ :param ddt: time-delay distance (physical Mpc) :param mu_intrinsic: intrinsic brightness of the source (already incorporating the inverse MST transform) :return: log likelihood of the measured magnified images given the source brightness """ model_vector, cov_tot = self._model_cov(ddt, mu_intrinsic) # invert matrix try: cov_tot_inv = np.linalg.inv(cov_tot) except: return -np.inf # difference to data vector delta = self._data_vector - model_vector # evaluate likelihood lnlikelihood = -delta.dot(cov_tot_inv.dot(delta)) / 2.0 sign_det, lndet = np.linalg.slogdet(cov_tot) lnlikelihood -= 1 / 2.0 * (self.num_data * np.log(2 * np.pi) + lndet) return lnlikelihood
def _model_cov(self, ddt, mu_intrinsic): """Combined covariance matrix of the data and model when marginialized over the Gaussian model uncertainties in the Fermat potential and magnification. :param ddt: time-delay distance (physical Mpc) :param mu_intrinsic: intrinsic brightness of the source (already incorporating the inverse MST transform) :return: model vector, combined covariance matrix """ # compute model predicted magnified image amplitude and time delay amp_intrinsic = magnitude2cps( magnitude=mu_intrinsic, magnitude_zero_point=self._magnitude_zero_point ) model_scale = np.append( ddt * self._fermat_unit_conversion * np.ones(self._n_td), amp_intrinsic * np.ones(self._n_amp), ) model_vector = model_scale * self._model_tot # scale model covariance matrix with model_scale vector (in quadrature) cov_model = model_scale * (self._cov_model * model_scale).T # combine data and model covariance matrix cov_tot = self._cov_data + cov_model return model_vector, cov_tot