import numpy as np
from lenstronomy.PointSource.Types.base_ps import PSBase, _expand_to_array
__all__ = ['LensedPositions']
[docs]class LensedPositions(PSBase):
"""
class of a a lensed point source parameterized as the (multiple) observed image positions
Name within the PointSource module: 'LENSED_POSITION'
parameters: ra_image, dec_image, point_amp
If fixed_magnification=True, than 'source_amp' is a parameter instead of 'point_amp'
"""
# def __init__(self, lens_model=None, fixed_magnification=False, additional_image=False):
# super(LensedPositions, self).__init__(lens_model=lens_model, fixed_magnification=fixed_magnification,
# additional_image=additional_image)
[docs] def image_position(self, kwargs_ps, kwargs_lens=None, magnification_limit=None, kwargs_lens_eqn_solver=None):
"""
on-sky image positions
:param kwargs_ps: keyword arguments of the point source model
:param kwargs_lens: keyword argument list of the lens model(s), only used when requiring the lens equation
solver
:param magnification_limit: float >0 or None, if float is set and additional images are computed, only those
images will be computed that exceed the lensing magnification (absolute value) limit
:param kwargs_lens_eqn_solver: keyword arguments specifying the numerical settings for the lens equation solver
see LensEquationSolver() class for details
:return: image positions in x, y as arrays
"""
if self._additional_image is True:
if kwargs_lens_eqn_solver is None:
kwargs_lens_eqn_solver = {}
ra_source, dec_source = self.source_position(kwargs_ps, kwargs_lens)
ra_image, dec_image = self._solver.image_position_from_source(ra_source, dec_source, kwargs_lens,
magnification_limit=magnification_limit,
**kwargs_lens_eqn_solver)
else:
ra_image = kwargs_ps['ra_image']
dec_image = kwargs_ps['dec_image']
return np.array(ra_image), np.array(dec_image)
[docs] def source_position(self, kwargs_ps, kwargs_lens=None):
"""
original source position (prior to lensing)
:param kwargs_ps: point source keyword arguments
:param kwargs_lens: lens model keyword argument list (required to ray-trace back in the source plane)
:return: x, y position (as numpy arrays)
"""
ra_image = kwargs_ps['ra_image']
dec_image = kwargs_ps['dec_image']
x_source, y_source = self._lens_model.ray_shooting(ra_image, dec_image, kwargs_lens)
x_source = np.mean(x_source)
y_source = np.mean(y_source)
return np.array(x_source), np.array(y_source)
[docs] def image_amplitude(self, kwargs_ps, kwargs_lens=None, x_pos=None, y_pos=None, magnification_limit=None,
kwargs_lens_eqn_solver=None):
"""
image brightness amplitudes
:param kwargs_ps: keyword arguments of the point source model
:param kwargs_lens: keyword argument list of the lens model(s), only used when requiring the lens equation
solver
:param x_pos: pre-computed image position (no lens equation solver applied)
:param y_pos: pre-computed image position (no lens equation solver applied)
:param magnification_limit: float >0 or None, if float is set and additional images are computed, only those
images will be computed that exceed the lensing magnification (absolute value) limit
:param kwargs_lens_eqn_solver: keyword arguments specifying the numerical settings for the lens equation solver
see LensEquationSolver() class for details
:return: array of image amplitudes
"""
if self._fixed_magnification:
if x_pos is not None and y_pos is not None:
ra_image, dec_image = x_pos, y_pos
else:
ra_image, dec_image = self.image_position(kwargs_ps, kwargs_lens,
magnification_limit=magnification_limit,
kwargs_lens_eqn_solver=kwargs_lens_eqn_solver)
mag = self._lens_model.magnification(ra_image, dec_image, kwargs_lens)
point_amp = kwargs_ps['source_amp'] * np.abs(mag)
else:
point_amp = kwargs_ps['point_amp']
if x_pos is not None:
point_amp = _expand_to_array(point_amp, len(x_pos))
return np.array(point_amp)
[docs] def source_amplitude(self, kwargs_ps, kwargs_lens=None):
"""
intrinsic brightness amplitude of point source
When brightnesses are defined in magnified on-sky positions, the intrinsic brightness is computed as the mean
in the magnification corrected image position brightnesses.
:param kwargs_ps: keyword arguments of the point source model
:param kwargs_lens: keyword argument list of the lens model(s), used when brightness are defined in
magnified on-sky positions
:return: brightness amplitude (as numpy array)
"""
if self._fixed_magnification:
source_amp = kwargs_ps['source_amp']
else:
ra_image, dec_image = kwargs_ps['ra_image'], kwargs_ps['dec_image']
mag = self._lens_model.magnification(ra_image, dec_image, kwargs_lens)
point_amp = kwargs_ps['point_amp']
source_amp = np.mean(np.array(point_amp) / np.array(np.abs(mag)))
return np.array(source_amp)