def test_ray_shooting_partial(self):
z_source = 1.5
lens_model_list = ['SIS', 'SIS', 'SIS']
sis1 = {'theta_E': 1., 'center_x': 0, 'center_y': 0}
sis2 = {'theta_E': .2, 'center_x': 0.5, 'center_y': 0}
sis3 = {'theta_E': .1, 'center_x': 0, 'center_y': 0.5}
z1 = 0.1
z2 = 0.5
z3 = 0.7
redshift_list = [z1, z2, z3]
kwargs_lens = [sis1, sis2, sis3]
lensModel = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
lensModel_2 = LensModel(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list, multi_plane=True)
multiplane_2 = lensModel_2.lens_model
intermediate_index = 1
theta_x, theta_y = 1., 1.
Tzsrc = lensModel._multi_plane_base._cosmo_bkg.T_xy(0, z_source)
z_intermediate = lensModel._multi_plane_base._lens_redshift_list[intermediate_index]
for lensmodel_class in [lensModel, multiplane_2]:
x_out, y_out, alpha_x_out, alpha_y_out = lensmodel_class.ray_shooting_partial(x=0, y=0, alpha_x=theta_x,
alpha_y=theta_y, z_start=0, z_stop=z_intermediate, kwargs_lens=kwargs_lens)
x_out_full_0 = x_out
y_out_full_0 = y_out
x_out, y_out, alpha_x_out, alpha_y_out = lensmodel_class.ray_shooting_partial(x=x_out, y=y_out, alpha_x=alpha_x_out,
alpha_y=alpha_y_out, z_start=z_intermediate,
z_stop=z_source,
kwargs_lens=kwargs_lens)
x_out_full_0 = np.append(x_out_full_0, x_out)
y_out_full_0 = np.append(y_out_full_0, y_out)
x_out_full, y_out_full, redshifts, tzlist = lensmodel_class.ray_shooting_partial_steps(x=0, y=0, alpha_x=theta_x,
alpha_y=theta_y, z_start=0, z_stop=z_source, kwargs_lens=kwargs_lens)
npt.assert_almost_equal(x_out_full_0[0], x_out_full[intermediate_index+1])
npt.assert_almost_equal(x_out_full_0[-1], x_out_full[-1])
npt.assert_almost_equal(y_out_full_0[0], y_out_full[intermediate_index+1])
npt.assert_almost_equal(y_out_full_0[-1], y_out_full[-1])
npt.assert_almost_equal(tzlist[0], lensModel._multi_plane_base._cosmo_bkg.T_xy(0, redshifts[0]))
beta_x, beta_y = lensModel._co_moving2angle_source(x_out, y_out)
beta_x_true, beta_y_true = lensmodel_class.ray_shooting(theta_x, theta_y, kwargs_lens)
npt.assert_almost_equal(beta_x, beta_x_true, decimal=8)
npt.assert_almost_equal(beta_y, beta_y_true, decimal=8)
T_ij_start = lensModel._multi_plane_base._cosmo_bkg.T_xy(z_observer=0, z_source=0.1)
T_ij_end = lensModel._multi_plane_base._cosmo_bkg.T_xy(z_observer=0.7, z_source=1.5)
x_out, y_out, alpha_x_out, alpha_y_out = lensmodel_class.ray_shooting_partial(x=0, y=0, alpha_x=theta_x,
alpha_y=theta_y, z_start=0, z_stop=z_source, kwargs_lens=kwargs_lens,
T_ij_start=T_ij_start, T_ij_end=T_ij_end)
beta_x, beta_y = x_out/Tzsrc, y_out/Tzsrc
npt.assert_almost_equal(beta_x, beta_x_true, decimal=8)
npt.assert_almost_equal(beta_y, beta_y_true, decimal=8)
def test_sis_travel_time_new(self):
z_source = 1.5
z_lens = 0.5
lens_model_list = ['SIS', 'SIS']
redshift_list = [z_lens, 0.2]
lensModelMutli = MultiPlane(z_source=z_source,
lens_model_list=lens_model_list,
lens_redshift_list=redshift_list)
lensModel = LensModel(lens_model_list=lens_model_list)
kwargs_lens = [{
'theta_E': 1.,
'center_x': 0,
'center_y': 0
}, {
'theta_E': 0.,
'center_x': 0,
'center_y': 0
}]
dt = lensModelMutli.arrival_time(1., 0., kwargs_lens)
Dt = lensModelMutli._multi_plane_base._cosmo_bkg.ddt(z_lens=z_lens,
z_source=z_source)
fermat_pot = lensModel.fermat_potential(1, 0., kwargs_lens)
dt_simple = const.delay_arcsec2days(fermat_pot, Dt)
print(dt, dt_simple)
npt.assert_almost_equal(dt, dt_simple, decimal=8)
def test_raise(self):
with self.assertRaises(ValueError):
MultiPlaneBase(z_source_convention=1, lens_model_list=['SIS'], lens_redshift_list=[2])
with self.assertRaises(ValueError):
MultiPlaneBase(z_source_convention=1, lens_model_list=['SIS', 'SIS'], lens_redshift_list=[0.5])
with self.assertRaises(ValueError):
lens = MultiPlane(z_source_convention=1, z_source=1, lens_model_list=['SIS', 'SIS'], lens_redshift_list=[0.5, 0.8])
lens._check_raise(k=[1])
def test_empty(self):
z_source = 1.5
lens_model_list = []
redshift_list = []
lensModelMutli = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
kwargs_lens = []
f_xx_multi, f_xy_multi, f_yx_multi, f_yy_multi = lensModelMutli.hessian(1, 0, kwargs_lens, diff=0.000001)
npt.assert_almost_equal(0, f_xx_multi, decimal=5)
npt.assert_almost_equal(0, f_xy_multi, decimal=5)
npt.assert_almost_equal(0, f_yx_multi, decimal=5)
npt.assert_almost_equal(0, f_yy_multi, decimal=5)
def test_sis_ray_tracing(self):
z_source = 1.5
lens_model_list = ['SIS']
redshift_list = [0.5]
lensModelMutli = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
lensModel = LensModel(lens_model_list=lens_model_list)
kwargs_lens = [{'theta_E': 1, 'center_x': 0, 'center_y': 0}]
beta_x_simple, beta_y_simple = lensModel.ray_shooting(1, 0, kwargs_lens)
beta_x_multi, beta_y_multi = lensModelMutli.ray_shooting(1, 0, kwargs_lens)
npt.assert_almost_equal(beta_x_simple, beta_x_multi, decimal=10)
npt.assert_almost_equal(beta_y_simple, beta_y_multi, decimal=10)
npt.assert_almost_equal(beta_x_simple, 0, decimal=10)
npt.assert_almost_equal(beta_y_simple, 0, decimal=10)
def test_sis_hessian(self):
z_source = 1.5
lens_model_list = ['SIS']
redshift_list = [0.5]
lensModelMutli = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
lensModel = LensModel(lens_model_list=lens_model_list)
kwargs_lens = [{'theta_E': 1, 'center_x': 0, 'center_y': 0}]
f_xx_simple, f_xy_simple, f_yx_simple, f_yy_simple = lensModel.hessian(1, 0, kwargs_lens)
f_xx_multi, f_xy_multi, f_yx_multi, f_yy_multi = lensModelMutli.hessian(1, 0, kwargs_lens, diff=0.000001)
npt.assert_almost_equal(f_xx_simple, f_xx_multi, decimal=5)
npt.assert_almost_equal(f_xy_simple, f_xy_multi, decimal=5)
npt.assert_almost_equal(f_yx_simple, f_yx_multi, decimal=5)
npt.assert_almost_equal(f_yy_simple, f_yy_multi, decimal=5)
def test_sis_alpha(self):
z_source = 1.5
lens_model_list = ['SIS']
redshift_list = [0.5]
lensModelMutli = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
lensModel = LensModel(lens_model_list=lens_model_list)
kwargs_lens = [{'theta_E': 1, 'center_x': 0, 'center_y': 0}]
alpha_x_simple, alpha_y_simple = lensModel.alpha(1, 0, kwargs_lens)
alpha_x_multi, alpha_y_multi = lensModelMutli.alpha(1, 0, kwargs_lens)
npt.assert_almost_equal(alpha_x_simple, alpha_x_multi, decimal=8)
npt.assert_almost_equal(alpha_y_simple, alpha_y_multi, decimal=8)
sum_partial = np.sum(lensModelMutli._multi_plane_base._T_ij_list) + lensModelMutli._T_ij_stop
T_z_true = lensModelMutli._T_z_source
npt.assert_almost_equal(sum_partial, T_z_true, decimal=5)
def test_sis_ray_shooting(self):
z_source = 1.5
z_lens = 0.5
lens_model_list = ['SIS']
redshift_list = [z_lens]
lensModelMutli = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
lensModel = LensModel(lens_model_list=lens_model_list)
kwargs_lens = [{'theta_E': 1., 'center_x': 0, 'center_y': 0}]
beta_x, beta_y = lensModelMutli.ray_shooting(1., 0., kwargs_lens)
beta_x_single, beta_y_single = lensModel.ray_shooting(1, 0., kwargs_lens)
npt.assert_almost_equal(beta_x, beta_x_single, decimal=8)
npt.assert_almost_equal(beta_y, beta_y_single, decimal=8)
x, y = np.array([1.]), np.array([2.])
beta_x, beta_y = lensModelMutli.ray_shooting(x, y, kwargs_lens)
beta_x_single, beta_y_single = lensModel.ray_shooting(x, y, kwargs_lens)
npt.assert_almost_equal(beta_x, beta_x_single, decimal=8)
npt.assert_almost_equal(beta_y, beta_y_single, decimal=8)
def test_pseudo_multiplane(self):
z_source = 1.5
lens_model_list = ['SIS', 'SIS']
sis1 = {'theta_E': 1., 'center_x': 0, 'center_y': 0}
sis2 = {'theta_E': .2, 'center_x': 0.5, 'center_y': 0}
z1 = 0.5
z2 = 0.5
redshift_list = [z1, z2]
kwargs_lens = [sis1, sis2]
lensModelMulti = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
lensModelSingle = LensModel(lens_model_list=lens_model_list)
beta_x, beta_y = lensModelMulti.ray_shooting(1, 1, kwargs_lens)
beta_x_single, beta_y_single = lensModelSingle.ray_shooting(1, 1, kwargs_lens)
npt.assert_almost_equal(beta_x, beta_x_single, decimal=10)
npt.assert_almost_equal(beta_y, beta_y_single, decimal=10)
def __init__(self, lens_model_list, z_lens=None, z_source=None, lens_redshift_list=None, cosmo=None,
multi_plane=False, numerical_alpha_class=None, observed_convention_index=None, z_source_convention=None):
"""
:param lens_model_list: list of strings with lens model names
:param z_lens: redshift of the deflector (only considered when operating in single plane mode).
Is only needed for specific functions that require a cosmology.
:param z_source: redshift of the source: Needed in multi_plane option only,
not required for the core functionalities in the single plane mode.
:param lens_redshift_list: list of deflector redshift (corresponding to the lens model list),
only applicable in multi_plane mode.
:param cosmo: instance of the astropy cosmology class. If not specified, uses the default cosmology.
:param multi_plane: bool, if True, uses multi-plane mode. Default is False.
:param numerical_alpha_class: an instance of a custom class for use in NumericalAlpha() lens model
(see documentation in Profiles/numerical_alpha)
:param observed_convention_index: a list of lens indexes that correspond to observed positions on the sky, not
physical positions
:param z_source_convention: float, redshift of a source to define the reduced deflection angles of the lens
models. If None, 'z_source' is used.
"""
self.lens_model_list = lens_model_list
self.z_lens = z_lens
if z_source_convention is None:
z_source_convention = z_source
self.z_source = z_source
self._z_source_convention = z_source_convention
self.redshift_list = lens_redshift_list
if cosmo is None:
cosmo = default_cosmology.get()
self.cosmo = cosmo
self.multi_plane = multi_plane
if multi_plane is True:
if z_source is None:
raise ValueError('z_source needs to be set for multi-plane lens modelling.')
self.lens_model = MultiPlane(z_source, lens_model_list, lens_redshift_list, cosmo=cosmo,
numerical_alpha_class=numerical_alpha_class,
observed_convention_index=observed_convention_index,
z_source_convention=z_source_convention)
else:
self.lens_model = SinglePlane(lens_model_list, numerical_alpha_class=numerical_alpha_class)
if z_lens is not None and z_source is not None:
self._lensCosmo = LensCosmo(z_lens, z_source, cosmo=cosmo)
def __init__(self,
lens_model_list,
z_lens=None,
z_source=None,
lens_redshift_list=None,
cosmo=None,
multi_plane=False,
numerical_alpha_class=None):
"""
:param lens_model_list: list of strings with lens model names
:param z_lens: redshift of the deflector (only considered when operating in single plane mode).
Is only needed for specific functions that require a cosmology.
:param z_source: redshift of the source: Needed in multi_plane option only,
not required for the core functionalities in the single plane mode.
:param lens_redshift_list: list of deflector redshift (corresponding to the lens model list),
only applicable in multi_plane mode.
:param cosmo: instance of the astropy cosmology class. If not specified, uses the default cosmology.
:param multi_plane: bool, if True, uses multi-plane mode. Default is False.
:param numerical_alpha_class: an instance of a custom class for use in NumericalAlpha() lens model
(see documentation in Profiles/numerical_alpha)
"""
self.lens_model_list = lens_model_list
self.z_lens = z_lens
self.z_source = z_source
self.redshift_list = lens_redshift_list
self.cosmo = cosmo
self.multi_plane = multi_plane
if multi_plane is True:
self.lens_model = MultiPlane(
z_source,
lens_model_list,
lens_redshift_list,
cosmo=cosmo,
numerical_alpha_class=numerical_alpha_class)
else:
self.lens_model = SinglePlane(
lens_model_list, numerical_alpha_class=numerical_alpha_class)
if z_lens is not None and z_source is not None:
self._lensCosmo = LensCosmo(z_lens, z_source, cosmo=self.cosmo)
def test_random_ordering(self):
z_source = 1.5
lens_model_list = ['SIS', 'SIS', 'SIS']
sis1 = {'theta_E': 1., 'center_x': 0, 'center_y': 0}
sis2 = {'theta_E': .2, 'center_x': 0.5, 'center_y': 0}
sis3 = {'theta_E': .1, 'center_x': 0, 'center_y': 0.5}
z1 = 0.1
z2 = 0.5
z3 = 0.7
redshift_list = [z1, z2, z3]
kwargs_lens = [sis1, sis2, sis3]
lensModel = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
beta_x_1, beta_y_1 = lensModel.ray_shooting(1., 0., kwargs_lens)
redshift_list = [z3, z2, z1]
kwargs_lens = [sis3, sis2, sis1]
lensModel = MultiPlane(z_source=z_source, lens_model_list=lens_model_list, lens_redshift_list=redshift_list)
beta_x_2, beta_y_2 = lensModel.ray_shooting(1., 0., kwargs_lens)
npt.assert_almost_equal(beta_x_1, beta_x_2, decimal=8)
npt.assert_almost_equal(beta_y_1, beta_y_2, decimal=8)
def __init__(self,
lens_model_list,
z_lens=None,
z_source=None,
lens_redshift_list=None,
cosmo=None,
multi_plane=False,
numerical_alpha_class=None,
observed_convention_index=None,
z_source_convention=None,
cosmo_interp=False,
z_interp_stop=None,
num_z_interp=100):
"""
:param lens_model_list: list of strings with lens model names
:param z_lens: redshift of the deflector (only considered when operating in single plane mode).
Is only needed for specific functions that require a cosmology.
:param z_source: redshift of the source: Needed in multi_plane option only,
not required for the core functionalities in the single plane mode.
:param lens_redshift_list: list of deflector redshift (corresponding to the lens model list),
only applicable in multi_plane mode.
:param cosmo: instance of the astropy cosmology class. If not specified, uses the default cosmology.
:param multi_plane: bool, if True, uses multi-plane mode. Default is False.
:param numerical_alpha_class: an instance of a custom class for use in NumericalAlpha() lens model
(see documentation in Profiles/numerical_alpha)
:param observed_convention_index: a list of indices, corresponding to the lens_model_list element with same
index, where the 'center_x' and 'center_y' kwargs correspond to observed (lensed) positions, not physical
positions. The code will compute the physical locations when performing computations
:param z_source_convention: float, redshift of a source to define the reduced deflection angles of the lens
models. If None, 'z_source' is used.
:param cosmo_interp: boolean (only employed in multi-plane mode), interpolates astropy.cosmology distances for
faster calls when accessing several lensing planes
:param z_interp_stop: (only in multi-plane with cosmo_interp=True); maximum redshift for distance interpolation
This number should be higher or equal the maximum of the source redshift and/or the z_source_convention
:param num_z_interp: (only in multi-plane with cosmo_interp=True); number of redshift bins for interpolating
distances
"""
self.lens_model_list = lens_model_list
self.z_lens = z_lens
self.z_source = z_source
self._z_source_convention = z_source_convention
self.redshift_list = lens_redshift_list
if cosmo is None:
from astropy.cosmology import default_cosmology
cosmo = default_cosmology.get()
self.cosmo = cosmo
self.multi_plane = multi_plane
if multi_plane is True:
if z_source is None:
raise ValueError(
'z_source needs to be set for multi-plane lens modelling.')
self.lens_model = MultiPlane(
z_source,
lens_model_list,
lens_redshift_list,
cosmo=cosmo,
numerical_alpha_class=numerical_alpha_class,
observed_convention_index=observed_convention_index,
z_source_convention=z_source_convention,
cosmo_interp=cosmo_interp,
z_interp_stop=z_interp_stop,
num_z_interp=num_z_interp)
else:
self.lens_model = SinglePlane(
lens_model_list,
numerical_alpha_class=numerical_alpha_class,
lens_redshift_list=lens_redshift_list,
z_source_convention=z_source_convention)
if z_lens is not None and z_source is not None:
self._lensCosmo = LensCosmo(z_lens, z_source, cosmo=cosmo)
def test_ray_shooting_partial_2(self):
z_source = 1.5
lens_model_list = ['SIS', 'SIS', 'SIS', 'SIS']
sis1 = {'theta_E': 0.4, 'center_x': 0, 'center_y': 0}
sis2 = {'theta_E': .2, 'center_x': 0.5, 'center_y': 0}
sis3 = {'theta_E': .1, 'center_x': 0, 'center_y': 0.5}
sis4 = {'theta_E': 0.5, 'center_x': 0.1, 'center_y': 0.3}
lens_model_list_macro = ['SIS']
kwargs_macro = [{'theta_E': 1, 'center_x': 0, 'center_y': 0}]
zmacro = 0.5
z1 = 0.1
z2 = 0.5
z3 = 0.5
z4 = 0.7
redshift_list = [z1, z2, z3, z4]
kwargs_lens = [sis1, sis2, sis3, sis4]
kwargs_lens_full = kwargs_macro + kwargs_lens
lensModel_full = MultiPlane(
z_source=z_source,
lens_model_list=lens_model_list_macro + lens_model_list,
lens_redshift_list=[zmacro] + redshift_list)
lensModel_macro = MultiPlane(z_source=z_source,
lens_model_list=lens_model_list_macro,
lens_redshift_list=[zmacro])
lensModel = MultiPlane(z_source=z_source,
lens_model_list=lens_model_list,
lens_redshift_list=redshift_list)
theta_x, theta_y = 1., 1.
x_subs, y_subs, alpha_x_subs, alpha_y_subs = lensModel.ray_shooting_partial(
x=0,
y=0,
alpha_x=theta_x,
alpha_y=theta_y,
z_start=0,
z_stop=zmacro,
kwargs_lens=kwargs_lens)
x_out, y_out, alpha_x_out, alpha_y_out = lensModel_macro.ray_shooting_partial(
x_subs,
y_subs,
alpha_x_subs,
alpha_y_subs,
zmacro,
zmacro,
kwargs_macro,
include_z_start=True)
npt.assert_almost_equal(x_subs, x_out)
npt.assert_almost_equal(y_subs, y_out)
x_full, y_full, alpha_x_full, alpha_y_full = lensModel_full.ray_shooting_partial(
0, 0, theta_x, theta_y, 0, zmacro, kwargs_lens_full)
npt.assert_almost_equal(x_full, x_out)
npt.assert_almost_equal(y_full, y_out)
npt.assert_almost_equal(alpha_x_full, alpha_x_out)
npt.assert_almost_equal(alpha_y_full, alpha_y_out)
x_src, y_src, _, _ = lensModel_full.ray_shooting_partial(
x=x_out,
y=y_out,
alpha_x=alpha_x_out,
alpha_y=alpha_y_out,
z_start=zmacro,
z_stop=z_source,
kwargs_lens=kwargs_lens_full)
beta_x, beta_y = lensModel._co_moving2angle_source(x_src, y_src)
beta_x_true, beta_y_true = lensModel_full.ray_shooting(
theta_x, theta_y, kwargs_lens_full)
npt.assert_almost_equal(beta_x, beta_x_true, decimal=8)
npt.assert_almost_equal(beta_y, beta_y_true, decimal=8)
def test_update_source_redshift(self):
z_source = 1.5
lens_model_list = ['SIS']
kwargs_lens = [{'theta_E': 1}]
redshift_list = [0.5]
lensModelMutli = MultiPlane(z_source=z_source,
lens_model_list=lens_model_list,
lens_redshift_list=redshift_list)
alpha_x, alpha_y = lensModelMutli.alpha(1, 0, kwargs_lens=kwargs_lens)
lensModelMutli.update_source_redshift(z_source=z_source)
alpha_x_new, alpha_y_new = lensModelMutli.alpha(
1, 0, kwargs_lens=kwargs_lens)
npt.assert_almost_equal(alpha_x / alpha_x_new, 1., decimal=8)
lensModelMutli.update_source_redshift(z_source=1.)
alpha_x_new, alpha_y_new = lensModelMutli.alpha(
1, 0, kwargs_lens=kwargs_lens)
assert alpha_x / alpha_x_new > 1
lensModelMutli.update_source_redshift(z_source=2.)
alpha_x_new, alpha_y_new = lensModelMutli.alpha(
1, 0, kwargs_lens=kwargs_lens)
assert alpha_x / alpha_x_new < 1
def test_foreground_shear(self):
"""
scenario: a shear field in the foreground of the main deflector is placed
we compute the expected shear on the lens plain and effectively model the same system in a single plane
configuration
We check for consistency of the two approaches and whether the specific redshift of the foreground shear field has
an impact on the arrival time surface
:return:
"""
z_source = 1.5
z_lens = 0.5
z_shear = 0.2
x, y = np.array([1., 0.]), np.array([0., 2.])
from astropy.cosmology import default_cosmology
from lenstronomy.Cosmo.background import Background
cosmo = default_cosmology.get()
cosmo_bkg = Background(cosmo)
e1, e2 = 0.01, 0.01 # shear terms caused by z_shear on z_source
lens_model_list = ['SIS', 'SHEAR']
redshift_list = [z_lens, z_shear]
lensModelMutli = MultiPlane(z_source=z_source,
lens_model_list=lens_model_list,
lens_redshift_list=redshift_list)
kwargs_lens_multi = [{
'theta_E': 1,
'center_x': 0,
'center_y': 0
}, {
'e1': e1,
'e2': e2
}]
alpha_x_multi, alpha_y_multi = lensModelMutli.alpha(
x, y, kwargs_lens_multi)
t_multi = lensModelMutli.arrival_time(x, y, kwargs_lens_multi)
dt_multi = t_multi[0] - t_multi[1]
physical_shear = cosmo_bkg.D_xy(0, z_source) / cosmo_bkg.D_xy(
z_shear, z_source)
foreground_factor = cosmo_bkg.D_xy(z_shear, z_lens) / cosmo_bkg.D_xy(
0, z_lens) * physical_shear
print(foreground_factor)
lens_model_simple_list = ['SIS', 'FOREGROUND_SHEAR', 'SHEAR']
kwargs_lens_single = [{
'theta_E': 1,
'center_x': 0,
'center_y': 0
}, {
'e1': e1 * foreground_factor,
'e2': e2 * foreground_factor
}, {
'e1': e1,
'e2': e2
}]
lensModel = LensModel(lens_model_list=lens_model_simple_list)
alpha_x_simple, alpha_y_simple = lensModel.alpha(
x, y, kwargs_lens_single)
npt.assert_almost_equal(alpha_x_simple, alpha_x_multi, decimal=8)
npt.assert_almost_equal(alpha_y_simple, alpha_y_multi, decimal=8)
ra_source, dec_source = lensModel.ray_shooting(x, y,
kwargs_lens_single)
ra_source_multi, dec_source_multi = lensModelMutli.ray_shooting(
x, y, kwargs_lens_multi)
npt.assert_almost_equal(ra_source, ra_source_multi, decimal=8)
npt.assert_almost_equal(dec_source, dec_source_multi, decimal=8)
fermat_pot = lensModel.fermat_potential(x, y, ra_source, dec_source,
kwargs_lens_single)
from lenstronomy.Cosmo.lens_cosmo import LensCosmo
lensCosmo = LensCosmo(z_lens, z_source, cosmo=cosmo)
Dt = lensCosmo.D_dt
print(lensCosmo.D_dt)
#t_simple = const.delay_arcsec2days(fermat_pot, Dt)
t_simple = lensCosmo.time_delay_units(fermat_pot)
dt_simple = t_simple[0] - t_simple[1]
print(t_simple, t_multi)
npt.assert_almost_equal(dt_simple / dt_multi, 1, decimal=2)
def test_ray_shooting_partial(self):
z_source = 1.5
lens_model_list = ['SIS', 'SIS', 'SIS']
sis1 = {'theta_E': 1., 'center_x': 0, 'center_y': 0}
sis2 = {'theta_E': .2, 'center_x': 0.5, 'center_y': 0}
sis3 = {'theta_E': .1, 'center_x': 0, 'center_y': 0.5}
z1 = 0.1
z2 = 0.5
z3 = 0.7
redshift_list = [z1, z2, z3]
kwargs_lens = [sis1, sis2, sis3]
lensModel = MultiPlane(z_source=z_source,
lens_model_list=lens_model_list,
lens_redshift_list=redshift_list)
intermediate_index = 1
theta_x, theta_y = 1., 1.
z_intermediate = lensModel._redshift_list[intermediate_index]
x_out, y_out, alpha_x_out, alpha_y_out = lensModel.ray_shooting_partial(
x=0,
y=0,
alpha_x=theta_x,
alpha_y=theta_y,
z_start=0,
z_stop=z_intermediate,
kwargs_lens=kwargs_lens)
x_out_full_0 = x_out
y_out_full_0 = y_out
x_out, y_out, alpha_x_out, alpha_y_out = lensModel.ray_shooting_partial(
x=x_out,
y=y_out,
alpha_x=alpha_x_out,
alpha_y=alpha_y_out,
z_start=z_intermediate,
z_stop=z_source,
kwargs_lens=kwargs_lens)
x_out_full_0 = np.append(x_out_full_0, x_out)
y_out_full_0 = np.append(y_out_full_0, y_out)
x_out_full, y_out_full, redshifts, tzlist = lensModel.ray_shooting_partial_steps(
x=0,
y=0,
alpha_x=theta_x,
alpha_y=theta_y,
z_start=0,
z_stop=z_source,
kwargs_lens=kwargs_lens)
npt.assert_almost_equal(x_out_full_0[0],
x_out_full[intermediate_index + 1])
npt.assert_almost_equal(x_out_full_0[-1], x_out_full[-1])
npt.assert_almost_equal(y_out_full_0[0],
y_out_full[intermediate_index + 1])
npt.assert_almost_equal(y_out_full_0[-1], y_out_full[-1])
npt.assert_almost_equal(redshifts[intermediate_index + 1],
lensModel._redshift_list[intermediate_index])
npt.assert_almost_equal(tzlist[0],
lensModel._cosmo_bkg.T_xy(0, redshifts[0]))
beta_x, beta_y = lensModel._co_moving2angle_source(x_out, y_out)
beta_x_true, beta_y_true = lensModel.ray_shooting(
theta_x, theta_y, kwargs_lens)
npt.assert_almost_equal(beta_x, beta_x_true, decimal=8)
npt.assert_almost_equal(beta_y, beta_y_true, decimal=8)
x_out, y_out, alpha_x_out, alpha_y_out = lensModel.ray_shooting_partial(
x=0,
y=0,
alpha_x=theta_x,
alpha_y=theta_y,
z_start=0,
z_stop=z_source,
kwargs_lens=kwargs_lens,
keep_range=True)
beta_x, beta_y = lensModel._co_moving2angle_source(x_out, y_out)
npt.assert_almost_equal(beta_x, beta_x_true, decimal=8)
npt.assert_almost_equal(beta_y, beta_y_true, decimal=8)
