def setup(self):
from lenstronomy.LensModel.Profiles.nie import NIE
from lenstronomy.LensModel.Profiles.spemd_smooth import SPEMD_SMOOTH
from lenstronomy.LensModel.Profiles.sis import SIS
self.nie = NIE()
self.spemd = SPEMD_SMOOTH()
self.sis = SIS()
def setup(self):
from lenstronomy.LensModel.Profiles.sie import SIE
from lenstronomy.LensModel.Profiles.spemd import SPEMD
from lenstronomy.LensModel.Profiles.nie import NIE
self.sie = SIE(NIE=False)
self.sie_nie = SIE(NIE=True)
self.spemd = SPEMD()
self.nie = NIE()
def setup(self):
from lenstronomy.LensModel.Profiles.sie import SIE
from lenstronomy.LensModel.Profiles.pemd import PEMD
from lenstronomy.LensModel.Profiles.nie import NIE
self.sie = SIE(NIE=False, suppress_fastell=True)
self.sie_nie = SIE(NIE=True)
self.spemd = PEMD(suppress_fastell=True)
self.nie = NIE()
def setup(self):
from lenstronomy.LensModel.Profiles.sie import SIE
from lenstronomy.LensModel.Profiles.epl import EPL
from lenstronomy.LensModel.Profiles.nie import NIE
self.sie = SIE(NIE=False)
self.sie_nie = SIE(NIE=True)
self.epl = EPL()
self.nie = NIE()
def test_function(self):
"""
:return:
"""
lens = NIE_lens()
light = NIE_light()
x = np.linspace(0.1, 10, 10)
e1, e2 = 0.1, 0
s = 0.2
kwargs_light = {'amp': 1., 'e1': e1, 'e2': e2, 's_scale': s}
kwargs_lens = {'theta_E': 1., 'e1': e1, 'e2': e2, 's_scale': s}
flux = light.function(x=x, y=1., **kwargs_light)
f_xx, f_yy, f_xy = lens.hessian(x=x, y=1., **kwargs_lens)
kappa = 1/2. * (f_xx + f_yy)
npt.assert_almost_equal(flux/flux[-1], kappa/kappa[-1], decimal=4)
def __init__(self, NIE=False):
self._nie = NIE
if NIE:
from lenstronomy.LensModel.Profiles.nie import NIE
self.profile = NIE()
else:
from lenstronomy.LensModel.Profiles.spemd import SPEMD
self.profile = SPEMD()
self._s_scale = 0.0000000001
self._gamma = 2
def __init__(self, NIE=True):
"""
:param NIE: bool, if True, is using the NIE analytic model. Otherwise it uses PEMD with gamma=2 from fastell4py
"""
self._nie = NIE
if NIE:
from lenstronomy.LensModel.Profiles.nie import NIE
self.profile = NIE()
else:
from lenstronomy.LensModel.Profiles.epl import EPL
self.profile = EPL()
self._s_scale = 0.0000000001
self._gamma = 2
super(SIE, self).__init__()
def __init__(self, NIE=True, suppress_fastell=False):
"""
:param NIE: bool, if True, is using the NIE analytic model. Otherwise it uses PEMD with gamma=2 from fastell4py
:param suppress_fastell: bool, if True, does not raise if fastell4py is not installed
"""
self._nie = NIE
if NIE:
from lenstronomy.LensModel.Profiles.nie import NIE
self.profile = NIE()
else:
from lenstronomy.LensModel.Profiles.pemd import PEMD
self.profile = PEMD(suppress_fastell=suppress_fastell)
self._s_scale = 0.0000000001
self._gamma = 2
super(SIE, self).__init__()
class TestChameleon(object):
"""
class to test the Moffat profile
"""
def setup(self):
self.chameleon = Chameleon()
self.nie = NIE()
def test_theta_E_convert(self):
w_c, w_t = 2, 1
theta_E_convert, w_c, w_t, s_scale_1, s_scale_2 = self.chameleon.param_convert(
alpha_1=1, w_c=w_c, w_t=w_t, e1=0, e2=0)
assert w_c == 1
assert w_t == 2
assert theta_E_convert == 0
def test_function(self):
"""
:return:
"""
x = np.linspace(0.1, 10, 10)
w_c, w_t = 0.5, 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_light = {
'alpha_1': 1.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
theta_E_convert, w_c, w_t, s_scale_1, s_scale_2 = self.chameleon.param_convert(
alpha_1=1, w_c=0.5, w_t=1., e1=e1, e2=e2)
kwargs_1 = {
'theta_E': theta_E_convert,
's_scale': s_scale_1,
'e1': e1,
'e2': e2
}
kwargs_2 = {
'theta_E': theta_E_convert,
's_scale': s_scale_2,
'e1': e1,
'e2': e2
}
f_ = self.chameleon.function(x=x, y=1., **kwargs_light)
f_1 = self.nie.function(x=x, y=1., **kwargs_1)
f_2 = self.nie.function(x=x, y=1., **kwargs_2)
npt.assert_almost_equal(f_, (f_1 - f_2), decimal=5)
def test_derivatives(self):
"""
:return:
"""
x = np.linspace(0.1, 10, 10)
w_c, w_t = 0.5, 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_light = {
'alpha_1': 1.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
theta_E_convert, w_c, w_t, s_scale_1, s_scale_2 = self.chameleon.param_convert(
alpha_1=1, w_c=0.5, w_t=1., e1=e1, e2=e2)
kwargs_1 = {
'theta_E': theta_E_convert,
's_scale': s_scale_1,
'e1': e1,
'e2': e2
}
kwargs_2 = {
'theta_E': theta_E_convert,
's_scale': s_scale_2,
'e1': e1,
'e2': e2
}
f_x, f_y = self.chameleon.derivatives(x=x, y=1., **kwargs_light)
f_x_1, f_y_1 = self.nie.derivatives(x=x, y=1., **kwargs_1)
f_x_2, f_y_2 = self.nie.derivatives(x=x, y=1., **kwargs_2)
npt.assert_almost_equal(f_x, (f_x_1 - f_x_2), decimal=5)
npt.assert_almost_equal(f_y, (f_y_1 - f_y_2), decimal=5)
f_x, f_y = self.chameleon.derivatives(x=1, y=0., **kwargs_light)
npt.assert_almost_equal(f_x, 1, decimal=1)
def test_hessian(self):
"""
:return:
"""
x = np.linspace(0.1, 10, 10)
w_c, w_t = 0.5, 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_light = {
'alpha_1': 1.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
theta_E_convert, w_c, w_t, s_scale_1, s_scale_2 = self.chameleon.param_convert(
alpha_1=1, w_c=0.5, w_t=1., e1=e1, e2=e2)
kwargs_1 = {
'theta_E': theta_E_convert,
's_scale': s_scale_1,
'e1': e1,
'e2': e2
}
kwargs_2 = {
'theta_E': theta_E_convert,
's_scale': s_scale_2,
'e1': e1,
'e2': e2
}
f_xx, f_xy, f_yx, f_yy = self.chameleon.hessian(x=x,
y=1.,
**kwargs_light)
f_xx_1, f_xy_1, f_yx_1, f_yy_1 = self.nie.hessian(x=x,
y=1.,
**kwargs_1)
f_xx_2, f_xy_2, f_yx_2, f_yy_2 = self.nie.hessian(x=x,
y=1.,
**kwargs_2)
npt.assert_almost_equal(f_xx, (f_xx_1 - f_xx_2), decimal=5)
npt.assert_almost_equal(f_yy, (f_yy_1 - f_yy_2), decimal=5)
npt.assert_almost_equal(f_xy, (f_xy_1 - f_xy_2), decimal=5)
npt.assert_almost_equal(f_yx, (f_yx_1 - f_yx_2), decimal=5)
def test_static(self):
x, y = 1., 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_light = {
'alpha_1': 1.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
f_ = self.chameleon.function(x, y, **kwargs_light)
self.chameleon.set_static(**kwargs_light)
f_static = self.chameleon.function(x, y, **kwargs_light)
npt.assert_almost_equal(f_, f_static, decimal=8)
self.chameleon.set_dynamic()
kwargs_light = {
'alpha_1': 2.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
f_dyn = self.chameleon.function(x, y, **kwargs_light)
assert f_dyn != f_static
def _import_class(self, lens_type, i, custom_class):
if lens_type == 'SHIFT':
from lenstronomy.LensModel.Profiles.alpha_shift import Shift
return Shift()
elif lens_type == 'SHEAR':
from lenstronomy.LensModel.Profiles.shear import Shear
return Shear()
elif lens_type == 'CONVERGENCE':
from lenstronomy.LensModel.Profiles.convergence import Convergence
return Convergence()
elif lens_type == 'FLEXION':
from lenstronomy.LensModel.Profiles.flexion import Flexion
return Flexion()
elif lens_type == 'POINT_MASS':
from lenstronomy.LensModel.Profiles.point_mass import PointMass
return PointMass()
elif lens_type == 'SIS':
from lenstronomy.LensModel.Profiles.sis import SIS
return SIS()
elif lens_type == 'SIS_TRUNCATED':
from lenstronomy.LensModel.Profiles.sis_truncate import SIS_truncate
return SIS_truncate()
elif lens_type == 'SIE':
from lenstronomy.LensModel.Profiles.sie import SIE
return SIE()
elif lens_type == 'SPP':
from lenstronomy.LensModel.Profiles.spp import SPP
return SPP()
elif lens_type == 'NIE':
from lenstronomy.LensModel.Profiles.nie import NIE
return NIE()
elif lens_type == 'NIE_SIMPLE':
from lenstronomy.LensModel.Profiles.nie import NIE_simple
return NIE_simple()
elif lens_type == 'CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import Chameleon
return Chameleon()
elif lens_type == 'DOUBLE_CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import DoubleChameleon
return DoubleChameleon()
elif lens_type == 'SPEP':
from lenstronomy.LensModel.Profiles.spep import SPEP
return SPEP()
elif lens_type == 'SPEMD':
from lenstronomy.LensModel.Profiles.spemd import SPEMD
return SPEMD()
elif lens_type == 'SPEMD_SMOOTH':
from lenstronomy.LensModel.Profiles.spemd_smooth import SPEMD_SMOOTH
return SPEMD_SMOOTH()
elif lens_type == 'NFW':
from lenstronomy.LensModel.Profiles.nfw import NFW
return NFW()
elif lens_type == 'NFW_ELLIPSE':
from lenstronomy.LensModel.Profiles.nfw_ellipse import NFW_ELLIPSE
return NFW_ELLIPSE()
elif lens_type == 'TNFW':
from lenstronomy.LensModel.Profiles.tnfw import TNFW
return TNFW()
elif lens_type == 'CNFW':
from lenstronomy.LensModel.Profiles.cnfw import CNFW
return CNFW()
elif lens_type == 'SERSIC':
from lenstronomy.LensModel.Profiles.sersic import Sersic
return Sersic()
elif lens_type == 'SERSIC_ELLIPSE':
from lenstronomy.LensModel.Profiles.sersic_ellipse import SersicEllipse
return SersicEllipse()
elif lens_type == 'PJAFFE':
from lenstronomy.LensModel.Profiles.p_jaffe import PJaffe
return PJaffe()
elif lens_type == 'PJAFFE_ELLIPSE':
from lenstronomy.LensModel.Profiles.p_jaffe_ellipse import PJaffe_Ellipse
return PJaffe_Ellipse()
elif lens_type == 'HERNQUIST':
from lenstronomy.LensModel.Profiles.hernquist import Hernquist
return Hernquist()
elif lens_type == 'HERNQUIST_ELLIPSE':
from lenstronomy.LensModel.Profiles.hernquist_ellipse import Hernquist_Ellipse
return Hernquist_Ellipse()
elif lens_type == 'GAUSSIAN':
from lenstronomy.LensModel.Profiles.gaussian_potential import Gaussian
return Gaussian()
elif lens_type == 'GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.gaussian_kappa import GaussianKappa
return GaussianKappa()
elif lens_type == 'GAUSSIAN_KAPPA_ELLIPSE':
from lenstronomy.LensModel.Profiles.gaussian_kappa_ellipse import GaussianKappaEllipse
return GaussianKappaEllipse()
elif lens_type == 'MULTI_GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappa
return MultiGaussianKappa()
elif lens_type == 'MULTI_GAUSSIAN_KAPPA_ELLIPSE':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappaEllipse
return MultiGaussianKappaEllipse()
elif lens_type == 'INTERPOL':
from lenstronomy.LensModel.Profiles.interpol import Interpol
return Interpol(grid=False, min_grid_number=100)
elif lens_type == 'INTERPOL_SCALED':
from lenstronomy.LensModel.Profiles.interpol import InterpolScaled
return InterpolScaled()
elif lens_type == 'SHAPELETS_POLAR':
from lenstronomy.LensModel.Profiles.shapelet_pot_polar import PolarShapelets
return PolarShapelets()
elif lens_type == 'SHAPELETS_CART':
from lenstronomy.LensModel.Profiles.shapelet_pot_cartesian import CartShapelets
return CartShapelets()
elif lens_type == 'DIPOLE':
from lenstronomy.LensModel.Profiles.dipole import Dipole
return Dipole()
elif lens_type == 'FOREGROUND_SHEAR':
from lenstronomy.LensModel.Profiles.shear import Shear
self._foreground_shear = True
self._foreground_shear_idex = i
return Shear()
elif lens_type == 'coreBURKERT':
from lenstronomy.LensModel.Profiles.coreBurkert import coreBurkert
return coreBurkert()
elif lens_type == 'NumericalAlpha':
from lenstronomy.LensModel.Profiles.numerical_deflections import NumericalAlpha
return NumericalAlpha(custom_class[i])
else:
raise ValueError('%s is not a valid lens model' % lens_type)
def __init__(self):
self.nie = NIE()
class TestEPL(object):
"""
tests the Gaussian methods
"""
def setup(self):
from lenstronomy.LensModel.Profiles.epl import EPL
self.EPL = EPL()
from lenstronomy.LensModel.Profiles.nie import NIE
self.NIE = NIE()
def test_function(self):
phi_E = 1.
t = 1.
q = 0.999
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = np.array([1., 2])
y = np.array([2, 0])
values = self.EPL.function(x, y, phi_E, e1, e2, t)
values_nie = self.NIE.function(x, y, phi_E, e1, e2, 0.)
delta_f = values[0] - values[1]
delta_f_nie = values_nie[0] - values_nie[1]
npt.assert_almost_equal(delta_f, delta_f_nie, decimal=5)
q = 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = np.array([1., 2])
y = np.array([2, 0])
values = self.EPL.function(x, y, phi_E, e1, e2, t)
values_nie = self.NIE.function(x, y, phi_E, e1, e2, 0.)
delta_f = values[0] - values[1]
delta_f_nie = values_nie[0] - values_nie[1]
npt.assert_almost_equal(delta_f, delta_f_nie, decimal=5)
q = 0.4
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = np.array([1., 2])
y = np.array([2, 0])
values = self.EPL.function(x, y, phi_E, e1, e2, t)
values_nie = self.NIE.function(x, y, phi_E, e1, e2, 0.)
delta_f = values[0] - values[1]
delta_f_nie = values_nie[0] - values_nie[1]
npt.assert_almost_equal(delta_f, delta_f_nie, decimal=5)
def test_derivatives(self):
x = np.array([1])
y = np.array([2])
phi_E = 1.
t = 1.
q = 1.
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.EPL.derivatives(x, y, phi_E, e1, e2, t)
f_x_nie, f_y_nie = self.NIE.derivatives(x, y, phi_E, e1, e2, 0.)
npt.assert_almost_equal(f_x, f_x_nie, decimal=4)
npt.assert_almost_equal(f_y, f_y_nie, decimal=4)
q = 0.7
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.EPL.derivatives(x, y, phi_E, e1, e2, t)
f_x_nie, f_y_nie = self.NIE.derivatives(x, y, phi_E, e1, e2, 0.)
npt.assert_almost_equal(f_x, f_x_nie, decimal=4)
npt.assert_almost_equal(f_y, f_y_nie, decimal=4)
def test_hessian(self):
x = np.array([1.])
y = np.array([2.])
phi_E = 1.
t = 1.
q = 0.9
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_xx, f_yy, f_xy = self.EPL.hessian(x, y, phi_E, e1, e2, t)
f_xx_nie, f_yy_nie, f_xy_nie = self.NIE.hessian(
x, y, phi_E, e1, e2, 0.)
npt.assert_almost_equal(f_xx, f_xx_nie, decimal=4)
npt.assert_almost_equal(f_yy, f_yy_nie, decimal=4)
npt.assert_almost_equal(f_xy, f_xy_nie, decimal=4)
def test_static(self):
x, y = 1., 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_lens = {'theta_E': 1., 't': 1.5, 'e1': e1, 'e2': e2}
f_ = self.EPL.function(x, y, **kwargs_lens)
self.EPL.set_static(**kwargs_lens)
f_static = self.EPL.function(x, y, **kwargs_lens)
npt.assert_almost_equal(f_, f_static, decimal=8)
self.EPL.set_dynamic()
kwargs_lens = {'theta_E': 2., 't': 0.5, 'e1': e1, 'e2': e2}
f_dyn = self.EPL.function(x, y, **kwargs_lens)
assert f_dyn != f_static
def setup(self):
self.chameleon = Chameleon()
self.nie = NIE()
def setup(self):
from lenstronomy.LensModel.Profiles.spemd import SPEMD
self.SPEMD = SPEMD(suppress_fastell=True)
from lenstronomy.LensModel.Profiles.nie import NIE
self.NIE = NIE()
def setup(self):
self.nie = NIE()
self.spemd = SPEMD(suppress_fastell=True)
self.sis = SIS()
def __init__(self, lens_model_list, **kwargs):
"""
:param lens_model_list: list of strings with lens model names
:param foreground_shear: bool, when True, models a foreground non-linear shear distortion
"""
self.func_list = []
self._foreground_shear = False
for i, lens_type in enumerate(lens_model_list):
if lens_type == 'SHEAR':
from lenstronomy.LensModel.Profiles.external_shear import ExternalShear
self.func_list.append(ExternalShear())
elif lens_type == 'CONVERGENCE':
from lenstronomy.LensModel.Profiles.mass_sheet import MassSheet
self.func_list.append(MassSheet())
elif lens_type == 'FLEXION':
from lenstronomy.LensModel.Profiles.flexion import Flexion
self.func_list.append(Flexion())
elif lens_type == 'POINT_MASS':
from lenstronomy.LensModel.Profiles.point_mass import PointMass
self.func_list.append(PointMass())
elif lens_type == 'SIS':
from lenstronomy.LensModel.Profiles.sis import SIS
self.func_list.append(SIS())
elif lens_type == 'SIS_TRUNCATED':
from lenstronomy.LensModel.Profiles.sis_truncate import SIS_truncate
self.func_list.append(SIS_truncate())
elif lens_type == 'SIE':
from lenstronomy.LensModel.Profiles.sie import SIE
self.func_list.append(SIE())
elif lens_type == 'SPP':
from lenstronomy.LensModel.Profiles.spp import SPP
self.func_list.append(SPP())
elif lens_type == 'NIE':
from lenstronomy.LensModel.Profiles.nie import NIE
self.func_list.append(NIE())
elif lens_type == 'NIE_SIMPLE':
from lenstronomy.LensModel.Profiles.nie import NIE_simple
self.func_list.append(NIE_simple())
elif lens_type == 'CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import Chameleon
self.func_list.append(Chameleon())
elif lens_type == 'DOUBLE_CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import DoubleChameleon
self.func_list.append(DoubleChameleon())
elif lens_type == 'SPEP':
from lenstronomy.LensModel.Profiles.spep import SPEP
self.func_list.append(SPEP())
elif lens_type == 'SPEMD':
from lenstronomy.LensModel.Profiles.spemd import SPEMD
self.func_list.append(SPEMD())
elif lens_type == 'SPEMD_SMOOTH':
from lenstronomy.LensModel.Profiles.spemd_smooth import SPEMD_SMOOTH
self.func_list.append(SPEMD_SMOOTH())
elif lens_type == 'NFW':
from lenstronomy.LensModel.Profiles.nfw import NFW
self.func_list.append(NFW(**kwargs))
elif lens_type == 'NFW_ELLIPSE':
from lenstronomy.LensModel.Profiles.nfw_ellipse import NFW_ELLIPSE
self.func_list.append(
NFW_ELLIPSE(interpol=False,
num_interp_X=1000,
max_interp_X=100))
elif lens_type == 'TNFW':
from lenstronomy.LensModel.Profiles.tnfw import TNFW
self.func_list.append(TNFW())
elif lens_type == 'SERSIC':
from lenstronomy.LensModel.Profiles.sersic import Sersic
self.func_list.append(Sersic())
elif lens_type == 'SERSIC_ELLIPSE':
from lenstronomy.LensModel.Profiles.sersic_ellipse import SersicEllipse
self.func_list.append(SersicEllipse())
elif lens_type == 'PJAFFE':
from lenstronomy.LensModel.Profiles.p_jaffe import PJaffe
self.func_list.append(PJaffe())
elif lens_type == 'PJAFFE_ELLIPSE':
from lenstronomy.LensModel.Profiles.p_jaffe_ellipse import PJaffe_Ellipse
self.func_list.append(PJaffe_Ellipse())
elif lens_type == 'HERNQUIST':
from lenstronomy.LensModel.Profiles.hernquist import Hernquist
self.func_list.append(Hernquist())
elif lens_type == 'HERNQUIST_ELLIPSE':
from lenstronomy.LensModel.Profiles.hernquist_ellipse import Hernquist_Ellipse
self.func_list.append(Hernquist_Ellipse())
elif lens_type == 'GAUSSIAN':
from lenstronomy.LensModel.Profiles.gaussian_potential import Gaussian
self.func_list.append(Gaussian())
elif lens_type == 'GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.gaussian_kappa import GaussianKappa
self.func_list.append(GaussianKappa())
elif lens_type == 'GAUSSIAN_KAPPA_ELLIPSE':
from lenstronomy.LensModel.Profiles.gaussian_kappa_ellipse import GaussianKappaEllipse
self.func_list.append(GaussianKappaEllipse())
elif lens_type == 'MULTI_GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappa
self.func_list.append(MultiGaussianKappa())
elif lens_type == 'MULTI_GAUSSIAN_KAPPA_ELLIPSE':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappaEllipse
self.func_list.append(MultiGaussianKappaEllipse())
elif lens_type == 'INTERPOL':
from lenstronomy.LensModel.Profiles.interpol import Interpol_func
self.func_list.append(
Interpol_func(grid=False, min_grid_number=100))
elif lens_type == 'INTERPOL_SCALED':
from lenstronomy.LensModel.Profiles.interpol import Interpol_func_scaled
self.func_list.append(
Interpol_func_scaled(grid=False, min_grid_number=100))
elif lens_type == 'SHAPELETS_POLAR':
from lenstronomy.LensModel.Profiles.shapelet_pot_polar import PolarShapelets
self.func_list.append(PolarShapelets())
elif lens_type == 'SHAPELETS_CART':
from lenstronomy.LensModel.Profiles.shapelet_pot_cartesian import CartShapelets
self.func_list.append(CartShapelets())
elif lens_type == 'DIPOLE':
from lenstronomy.LensModel.Profiles.dipole import Dipole
self.func_list.append(Dipole())
elif lens_type == 'FOREGROUND_SHEAR':
from lenstronomy.LensModel.Profiles.external_shear import ExternalShear
self.func_list.append(ExternalShear())
self._foreground_shear = True
self._foreground_shear_idex = i
else:
raise ValueError('%s is not a valid lens model' % lens_type)
self._model_list = lens_model_list
class TestEPLvsNIE(object):
"""
tests the Gaussian methods
"""
def setup(self):
from lenstronomy.LensModel.Profiles.epl import EPL
self.EPL = EPL()
from lenstronomy.LensModel.Profiles.nie import NIE
self.NIE = NIE()
def test_function(self):
phi_E = 1.
gamma = 2.
q = 0.999
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = np.array([1., 2])
y = np.array([2, 0])
values = self.EPL.function(x, y, phi_E, gamma, e1, e2)
values_nie = self.NIE.function(x, y, phi_E, e1, e2, 0.)
delta_f = values[0] - values[1]
delta_f_nie = values_nie[0] - values_nie[1]
npt.assert_almost_equal(delta_f, delta_f_nie, decimal=5)
q = 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = np.array([1., 2])
y = np.array([2, 0])
values = self.EPL.function(x, y, phi_E, gamma, e1, e2)
values_nie = self.NIE.function(x, y, phi_E, e1, e2, 0.)
delta_f = values[0] - values[1]
delta_f_nie = values_nie[0] - values_nie[1]
npt.assert_almost_equal(delta_f, delta_f_nie, decimal=5)
q = 0.4
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = np.array([1., 2])
y = np.array([2, 0])
values = self.EPL.function(x, y, phi_E, gamma, e1, e2)
values_nie = self.NIE.function(x, y, phi_E, e1, e2, 0.)
delta_f = values[0] - values[1]
delta_f_nie = values_nie[0] - values_nie[1]
npt.assert_almost_equal(delta_f, delta_f_nie, decimal=5)
def test_derivatives(self):
x = np.array([1])
y = np.array([2])
phi_E = 1.
gamma = 2.
q = 1.
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.EPL.derivatives(x, y, phi_E, gamma, e1, e2)
f_x_nie, f_y_nie = self.NIE.derivatives(x, y, phi_E, e1, e2, 0.)
npt.assert_almost_equal(f_x, f_x_nie, decimal=4)
npt.assert_almost_equal(f_y, f_y_nie, decimal=4)
q = 0.7
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.EPL.derivatives(x, y, phi_E, gamma, e1, e2)
f_x_nie, f_y_nie = self.NIE.derivatives(x, y, phi_E, e1, e2, 0.)
npt.assert_almost_equal(f_x, f_x_nie, decimal=4)
npt.assert_almost_equal(f_y, f_y_nie, decimal=4)
def test_hessian(self):
x = np.array([1.])
y = np.array([2.])
phi_E = 1.
gamma = 2.
q = 0.9
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_xx, f_xy, f_yx, f_yy = self.EPL.hessian(x, y, phi_E, gamma, e1, e2)
f_xx_nie, f_xy_nie, f_yx_nie, f_yy_nie = self.NIE.hessian(x, y, phi_E, e1, e2, 0.)
npt.assert_almost_equal(f_xx, f_xx_nie, decimal=4)
npt.assert_almost_equal(f_yy, f_yy_nie, decimal=4)
npt.assert_almost_equal(f_xy, f_xy_nie, decimal=4)
npt.assert_almost_equal(f_xy, f_yx, decimal=8)
def test_density_lens(self):
r = 1
kwargs = {'theta_E': 1, 'gamma': 2, 'e1': 0, 'e2': 0}
rho = self.EPL.density_lens(r, **kwargs)
from lenstronomy.LensModel.Profiles.spep import SPEP
spep = SPEP()
rho_spep = spep.density_lens(r, **kwargs)
npt.assert_almost_equal(rho, rho_spep, decimal=7)
def test_mass_3d_lens(self):
r = 1
kwargs = {'theta_E': 1, 'gamma': 2, 'e1': 0, 'e2': 0}
rho = self.EPL.mass_3d_lens(r, **kwargs)
from lenstronomy.LensModel.Profiles.spep import SPEP
spep = SPEP()
rho_spep = spep.mass_3d_lens(r, **kwargs)
npt.assert_almost_equal(rho, rho_spep, decimal=7)
def test_static(self):
x, y = 1., 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_lens = {'theta_E': 1., 'gamma': 1.5, 'e1': e1, 'e2': e2}
f_ = self.EPL.function(x, y, **kwargs_lens)
self.EPL.set_static(**kwargs_lens)
f_static = self.EPL.function(x, y, **kwargs_lens)
npt.assert_almost_equal(f_, f_static, decimal=8)
self.EPL.set_dynamic()
kwargs_lens = {'theta_E': 2., 'gamma': 1.9, 'e1': e1, 'e2': e2}
f_dyn = self.EPL.function(x, y, **kwargs_lens)
assert f_dyn != f_static
def test_regularization(self):
phi_E = 1.
gamma = 2.
q = 1.
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = 0.
y = 0.
f_x, f_y = self.EPL.derivatives(x, y, phi_E, gamma, e1, e2)
npt.assert_almost_equal(f_x, 0.)
npt.assert_almost_equal(f_y, 0.)
x = 0.
y = 0.
f_xx, f_xy, f_yx, f_yy = self.EPL.hessian(x, y, phi_E, gamma, e1, e2)
assert f_xx > 10 ** 5
assert f_yy > 10 ** 5
#npt.assert_almost_equal(f_xx, 10**10)
#npt.assert_almost_equal(f_yy, 10**10)
npt.assert_almost_equal(f_xy, 0)
npt.assert_almost_equal(f_yx, 0)
def __init__(self, static=False):
self._nie_1 = NIE()
self._nie_2 = NIE()
super(Chameleon, self).__init__()
self._static = static
class Chameleon(LensProfileBase):
"""
class of the Chameleon model (See Suyu+2014) an elliptical truncated double isothermal profile
"""
param_names = ['alpha_1', 'w_c', 'w_t', 'e1', 'e2', 'center_x', 'center_y']
lower_limit_default = {'alpha_1': 0, 'w_c': 0, 'w_t': 0, 'e1': -0.8, 'e2': -0.8, 'center_x': -100, 'center_y': -100}
upper_limit_default = {'alpha_1': 100, 'w_c': 100, 'w_t': 100, 'e1': 0.8, 'e2': 0.8, 'center_x': 100, 'center_y': 100}
def __init__(self, static=False):
self._nie_1 = NIE()
self._nie_2 = NIE()
super(Chameleon, self).__init__()
self._static = static
def function(self, x, y, alpha_1, w_c, w_t, e1, e2, center_x=0, center_y=0):
"""
:param x: ra-coordinate
:param y: dec-coordinate
:param alpha_1: deflection angle at 1 (arcseconds) from the center
:param w_c: see Suyu+2014
:param w_t: see Suyu+2014
:param e1: ellipticity parameter
:param e2: ellipticity parameter
:param center_x: ra center
:param center_y: dec center
:return: lensing potential
"""
theta_E_conv, w_c, w_t, s_scale_1, s_scale_2 = self.param_convert(alpha_1, w_c, w_t, e1, e2)
f_1 = self._nie_1.function(x, y, theta_E_conv, e1, e2, s_scale_1, center_x, center_y)
f_2 = self._nie_2.function(x, y, theta_E_conv, e1, e2, s_scale_2, center_x, center_y)
f_ = f_1 - f_2
return f_
def derivatives(self, x, y, alpha_1, w_c, w_t, e1, e2, center_x=0, center_y=0):
"""
:param x: ra-coordinate
:param y: dec-coordinate
:param alpha_1: deflection angle at 1 (arcseconds) from the center
:param w_c: see Suyu+2014
:param w_t: see Suyu+2014
:param e1: ellipticity parameter
:param e2: ellipticity parameter
:param center_x: ra center
:param center_y: dec center
:return: deflection angles (RA, DEC)
"""
theta_E_conv, w_c, w_t, s_scale_1, s_scale_2 = self.param_convert(alpha_1, w_c, w_t, e1, e2)
f_x_1, f_y_1 = self._nie_1.derivatives(x, y, theta_E_conv, e1, e2, s_scale_1, center_x, center_y)
f_x_2, f_y_2 = self._nie_2.derivatives(x, y, theta_E_conv, e1, e2, s_scale_2, center_x, center_y)
f_x = f_x_1 - f_x_2
f_y = f_y_1 - f_y_2
return f_x, f_y
def hessian(self, x, y, alpha_1, w_c, w_t, e1, e2, center_x=0, center_y=0):
"""
:param x: ra-coordinate
:param y: dec-coordinate
:param alpha_1: deflection angle at 1 (arcseconds) from the center
:param w_c: see Suyu+2014
:param w_t: see Suyu+2014
:param e1: ellipticity parameter
:param e2: ellipticity parameter
:param center_x: ra center
:param center_y: dec center
:return: second derivatives of the lensing potential (Hessian: f_xx, f_xy, f_yx, f_yy)
"""
theta_E_conv, w_c, w_t, s_scale_1, s_scale_2 = self.param_convert(alpha_1, w_c, w_t, e1, e2)
f_xx_1, f_xy_1, f_yx_1, f_yy_1 = self._nie_1.hessian(x, y, theta_E_conv, e1, e2, s_scale_1, center_x, center_y)
f_xx_2, f_xy_2, f_yx_2, f_yy_2 = self._nie_2.hessian(x, y, theta_E_conv, e1, e2, s_scale_2, center_x, center_y)
f_xx = f_xx_1 - f_xx_2
f_yy = f_yy_1 - f_yy_2
f_xy = f_xy_1 - f_xy_2
f_yx = f_yx_1 - f_yx_2
return f_xx, f_xy, f_yx, f_yy
def param_convert(self, alpha_1, w_c, w_t, e1, e2):
"""
convert the parameter alpha_1 (deflection angle one arcsecond from the center) into the
"Einstein radius" scale parameter of the two NIE profiles
:param alpha_1: deflection angle at 1 (arcseconds) from the center
:param w_c: see Suyu+2014
:param w_t: see Suyu+2014
:param e1: eccentricity modulus
:param ee: eccentricity modulus
:return:
"""
if self._static is True:
return self._theta_convert_static, self._w_c_static, self._w_t_stactic, self._s_scale_1_static, self._s_scale_2_static
return self._param_convert(alpha_1, w_c, w_t, e1, e2)
def _param_convert(self, alpha_1, w_c, w_t, e1, e2):
if not w_t >= w_c:
return 0, w_t, w_c, 1, 1
s_scale_1 = w_c
s_scale_2 = w_t
f_x_1, f_y_1 = self._nie_1.derivatives(1, 0, theta_E=1, e1=0, e2=0, s_scale=s_scale_1)
f_x_2, f_y_2 = self._nie_2.derivatives(1, 0, theta_E=1, e1=0, e2=0, s_scale=s_scale_2)
f_x = f_x_1 - f_x_2
theta_E_convert = alpha_1 / f_x
phi_G, q = param_util.ellipticity2phi_q(e1, e2)
s_scale_1 = np.sqrt(4 * w_c ** 2 / (1. + q) ** 2)
s_scale_2 = np.sqrt(4 * w_t ** 2 / (1. + q) ** 2)
return theta_E_convert, w_c, w_t, s_scale_1, s_scale_2
def set_static(self, alpha_1, w_c, w_t, e1, e2, center_x=0, center_y=0):
"""
:param logM:
:param concentration:
:param center_x:
:param center_y:
:return:
"""
self._static = True
self._theta_convert_static, self._w_c_static, self._w_t_stactic, self._s_scale_1_static, self._s_scale_2_static = self._param_convert(alpha_1, w_c, w_t, e1, e2)
self._nie_1.set_static(self._theta_convert_static, e1, e2, self._s_scale_1_static, center_x, center_y)
self._nie_2.set_static(self._theta_convert_static, e1, e2, self._s_scale_2_static, center_x, center_y)
def set_dynamic(self):
"""
:return:
"""
self._static = False
if hasattr(self, '_theta_convert_static'):
del self._theta_convert_static
if hasattr(self, '_w_c_static'):
del self._w_c_static
if hasattr(self, '_w_t_stactic'):
del self._w_t_stactic
if hasattr(self, '_s_scale_1_static'):
del self._s_scale_1_static
if hasattr(self, '_s_scale_2_static'):
del self._s_scale_2_static
self._nie_1.set_dynamic()
self._nie_2.set_dynamic()
def setup(self):
self.nie = NIE()
self.spemd = SPEMD_SMOOTH()
self.sis = SIS()
def setup(self):
from lenstronomy.LensModel.Profiles.epl import EPL
self.EPL = EPL()
from lenstronomy.LensModel.Profiles.nie import NIE
self.NIE = NIE()
def _import_class(lens_type,
custom_class,
kwargs_interp,
z_lens=None,
z_source=None):
"""
:param lens_type: string, lens model type
:param custom_class: custom class
:param z_lens: lens redshift # currently only used in NFW_MC model as this is redshift dependent
:param z_source: source redshift # currently only used in NFW_MC model as this is redshift dependent
:param kwargs_interp: interpolation keyword arguments specifying the numerics.
See description in the Interpolate() class. Only applicable for 'INTERPOL' and 'INTERPOL_SCALED' models.
:return: class instance of the lens model type
"""
if lens_type == 'SHIFT':
from lenstronomy.LensModel.Profiles.constant_shift import Shift
return Shift()
elif lens_type == 'NIE_POTENTIAL':
from lenstronomy.LensModel.Profiles.nie_potential import NIE_POTENTIAL
return NIE_POTENTIAL()
elif lens_type == 'CONST_MAG':
from lenstronomy.LensModel.Profiles.const_mag import ConstMag
return ConstMag()
elif lens_type == 'SHEAR':
from lenstronomy.LensModel.Profiles.shear import Shear
return Shear()
elif lens_type == 'SHEAR_GAMMA_PSI':
from lenstronomy.LensModel.Profiles.shear import ShearGammaPsi
return ShearGammaPsi()
elif lens_type == 'SHEAR_REDUCED':
from lenstronomy.LensModel.Profiles.shear import ShearReduced
return ShearReduced()
elif lens_type == 'CONVERGENCE':
from lenstronomy.LensModel.Profiles.convergence import Convergence
return Convergence()
elif lens_type == 'HESSIAN':
from lenstronomy.LensModel.Profiles.hessian import Hessian
return Hessian()
elif lens_type == 'FLEXION':
from lenstronomy.LensModel.Profiles.flexion import Flexion
return Flexion()
elif lens_type == 'FLEXIONFG':
from lenstronomy.LensModel.Profiles.flexionfg import Flexionfg
return Flexionfg()
elif lens_type == 'POINT_MASS':
from lenstronomy.LensModel.Profiles.point_mass import PointMass
return PointMass()
elif lens_type == 'SIS':
from lenstronomy.LensModel.Profiles.sis import SIS
return SIS()
elif lens_type == 'SIS_TRUNCATED':
from lenstronomy.LensModel.Profiles.sis_truncate import SIS_truncate
return SIS_truncate()
elif lens_type == 'SIE':
from lenstronomy.LensModel.Profiles.sie import SIE
return SIE()
elif lens_type == 'SPP':
from lenstronomy.LensModel.Profiles.spp import SPP
return SPP()
elif lens_type == 'NIE':
from lenstronomy.LensModel.Profiles.nie import NIE
return NIE()
elif lens_type == 'NIE_SIMPLE':
from lenstronomy.LensModel.Profiles.nie import NIEMajorAxis
return NIEMajorAxis()
elif lens_type == 'CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import Chameleon
return Chameleon()
elif lens_type == 'DOUBLE_CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import DoubleChameleon
return DoubleChameleon()
elif lens_type == 'TRIPLE_CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import TripleChameleon
return TripleChameleon()
elif lens_type == 'SPEP':
from lenstronomy.LensModel.Profiles.spep import SPEP
return SPEP()
elif lens_type == 'PEMD':
from lenstronomy.LensModel.Profiles.pemd import PEMD
return PEMD()
elif lens_type == 'SPEMD':
from lenstronomy.LensModel.Profiles.spemd import SPEMD
return SPEMD()
elif lens_type == 'EPL':
from lenstronomy.LensModel.Profiles.epl import EPL
return EPL()
elif lens_type == 'EPL_NUMBA':
from lenstronomy.LensModel.Profiles.epl_numba import EPL_numba
return EPL_numba()
elif lens_type == 'SPL_CORE':
from lenstronomy.LensModel.Profiles.splcore import SPLCORE
return SPLCORE()
elif lens_type == 'NFW':
from lenstronomy.LensModel.Profiles.nfw import NFW
return NFW()
elif lens_type == 'NFW_ELLIPSE':
from lenstronomy.LensModel.Profiles.nfw_ellipse import NFW_ELLIPSE
return NFW_ELLIPSE()
elif lens_type == 'NFW_ELLIPSE_GAUSS_DEC':
from lenstronomy.LensModel.Profiles.gauss_decomposition import NFWEllipseGaussDec
return NFWEllipseGaussDec()
elif lens_type == 'NFW_ELLIPSE_CSE':
from lenstronomy.LensModel.Profiles.nfw_ellipse_cse import NFW_ELLIPSE_CSE
return NFW_ELLIPSE_CSE()
elif lens_type == 'TNFW':
from lenstronomy.LensModel.Profiles.tnfw import TNFW
return TNFW()
elif lens_type == 'TNFW_ELLIPSE':
from lenstronomy.LensModel.Profiles.tnfw_ellipse import TNFW_ELLIPSE
return TNFW_ELLIPSE()
elif lens_type == 'CNFW':
from lenstronomy.LensModel.Profiles.cnfw import CNFW
return CNFW()
elif lens_type == 'CNFW_ELLIPSE':
from lenstronomy.LensModel.Profiles.cnfw_ellipse import CNFW_ELLIPSE
return CNFW_ELLIPSE()
elif lens_type == 'CTNFW_GAUSS_DEC':
from lenstronomy.LensModel.Profiles.gauss_decomposition import CTNFWGaussDec
return CTNFWGaussDec()
elif lens_type == 'NFW_MC':
from lenstronomy.LensModel.Profiles.nfw_mass_concentration import NFWMC
return NFWMC(z_lens=z_lens, z_source=z_source)
elif lens_type == 'SERSIC':
from lenstronomy.LensModel.Profiles.sersic import Sersic
return Sersic()
elif lens_type == 'SERSIC_ELLIPSE_POTENTIAL':
from lenstronomy.LensModel.Profiles.sersic_ellipse_potential import SersicEllipse
return SersicEllipse()
elif lens_type == 'SERSIC_ELLIPSE_KAPPA':
from lenstronomy.LensModel.Profiles.sersic_ellipse_kappa import SersicEllipseKappa
return SersicEllipseKappa()
elif lens_type == 'SERSIC_ELLIPSE_GAUSS_DEC':
from lenstronomy.LensModel.Profiles.gauss_decomposition import SersicEllipseGaussDec
return SersicEllipseGaussDec()
elif lens_type == 'PJAFFE':
from lenstronomy.LensModel.Profiles.p_jaffe import PJaffe
return PJaffe()
elif lens_type == 'PJAFFE_ELLIPSE':
from lenstronomy.LensModel.Profiles.p_jaffe_ellipse import PJaffe_Ellipse
return PJaffe_Ellipse()
elif lens_type == 'HERNQUIST':
from lenstronomy.LensModel.Profiles.hernquist import Hernquist
return Hernquist()
elif lens_type == 'HERNQUIST_ELLIPSE':
from lenstronomy.LensModel.Profiles.hernquist_ellipse import Hernquist_Ellipse
return Hernquist_Ellipse()
elif lens_type == 'HERNQUIST_ELLIPSE_CSE':
from lenstronomy.LensModel.Profiles.hernquist_ellipse_cse import HernquistEllipseCSE
return HernquistEllipseCSE()
elif lens_type == 'GAUSSIAN':
from lenstronomy.LensModel.Profiles.gaussian_potential import Gaussian
return Gaussian()
elif lens_type == 'GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.gaussian_kappa import GaussianKappa
return GaussianKappa()
elif lens_type == 'GAUSSIAN_ELLIPSE_KAPPA':
from lenstronomy.LensModel.Profiles.gaussian_ellipse_kappa import GaussianEllipseKappa
return GaussianEllipseKappa()
elif lens_type == 'GAUSSIAN_ELLIPSE_POTENTIAL':
from lenstronomy.LensModel.Profiles.gaussian_ellipse_potential import GaussianEllipsePotential
return GaussianEllipsePotential()
elif lens_type == 'MULTI_GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappa
return MultiGaussianKappa()
elif lens_type == 'MULTI_GAUSSIAN_KAPPA_ELLIPSE':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappaEllipse
return MultiGaussianKappaEllipse()
elif lens_type == 'INTERPOL':
from lenstronomy.LensModel.Profiles.interpol import Interpol
return Interpol(**kwargs_interp)
elif lens_type == 'INTERPOL_SCALED':
from lenstronomy.LensModel.Profiles.interpol import InterpolScaled
return InterpolScaled(**kwargs_interp)
elif lens_type == 'SHAPELETS_POLAR':
from lenstronomy.LensModel.Profiles.shapelet_pot_polar import PolarShapelets
return PolarShapelets()
elif lens_type == 'SHAPELETS_CART':
from lenstronomy.LensModel.Profiles.shapelet_pot_cartesian import CartShapelets
return CartShapelets()
elif lens_type == 'DIPOLE':
from lenstronomy.LensModel.Profiles.dipole import Dipole
return Dipole()
elif lens_type == 'CURVED_ARC_CONST':
from lenstronomy.LensModel.Profiles.curved_arc_const import CurvedArcConst
return CurvedArcConst()
elif lens_type == 'CURVED_ARC_CONST_MST':
from lenstronomy.LensModel.Profiles.curved_arc_const import CurvedArcConstMST
return CurvedArcConstMST()
elif lens_type == 'CURVED_ARC_SPP':
from lenstronomy.LensModel.Profiles.curved_arc_spp import CurvedArcSPP
return CurvedArcSPP()
elif lens_type == 'CURVED_ARC_SIS_MST':
from lenstronomy.LensModel.Profiles.curved_arc_sis_mst import CurvedArcSISMST
return CurvedArcSISMST()
elif lens_type == 'CURVED_ARC_SPT':
from lenstronomy.LensModel.Profiles.curved_arc_spt import CurvedArcSPT
return CurvedArcSPT()
elif lens_type == 'CURVED_ARC_TAN_DIFF':
from lenstronomy.LensModel.Profiles.curved_arc_tan_diff import CurvedArcTanDiff
return CurvedArcTanDiff()
elif lens_type == 'ARC_PERT':
from lenstronomy.LensModel.Profiles.arc_perturbations import ArcPerturbations
return ArcPerturbations()
elif lens_type == 'coreBURKERT':
from lenstronomy.LensModel.Profiles.coreBurkert import CoreBurkert
return CoreBurkert()
elif lens_type == 'CORED_DENSITY':
from lenstronomy.LensModel.Profiles.cored_density import CoredDensity
return CoredDensity()
elif lens_type == 'CORED_DENSITY_2':
from lenstronomy.LensModel.Profiles.cored_density_2 import CoredDensity2
return CoredDensity2()
elif lens_type == 'CORED_DENSITY_EXP':
from lenstronomy.LensModel.Profiles.cored_density_exp import CoredDensityExp
return CoredDensityExp()
elif lens_type == 'CORED_DENSITY_MST':
from lenstronomy.LensModel.Profiles.cored_density_mst import CoredDensityMST
return CoredDensityMST(profile_type='CORED_DENSITY')
elif lens_type == 'CORED_DENSITY_2_MST':
from lenstronomy.LensModel.Profiles.cored_density_mst import CoredDensityMST
return CoredDensityMST(profile_type='CORED_DENSITY_2')
elif lens_type == 'CORED_DENSITY_EXP_MST':
from lenstronomy.LensModel.Profiles.cored_density_mst import CoredDensityMST
return CoredDensityMST(profile_type='CORED_DENSITY_EXP')
elif lens_type == 'NumericalAlpha':
from lenstronomy.LensModel.Profiles.numerical_deflections import NumericalAlpha
return NumericalAlpha(custom_class)
elif lens_type == 'MULTIPOLE':
from lenstronomy.LensModel.Profiles.multipole import Multipole
return Multipole()
elif lens_type == 'CSE':
from lenstronomy.LensModel.Profiles.cored_steep_ellipsoid import CSE
return CSE()
elif lens_type == 'ElliSLICE':
from lenstronomy.LensModel.Profiles.elliptical_density_slice import ElliSLICE
return ElliSLICE()
elif lens_type == 'ULDM':
from lenstronomy.LensModel.Profiles.uldm import Uldm
return Uldm()
elif lens_type == 'CORED_DENSITY_ULDM_MST':
from lenstronomy.LensModel.Profiles.cored_density_mst import CoredDensityMST
return CoredDensityMST(profile_type='CORED_DENSITY_ULDM')
else:
raise ValueError(
'%s is not a valid lens model. Supported are: %s.' %
(lens_type, _SUPPORTED_MODELS))
class TestNIE(object):
"""
tests the Gaussian methods
"""
def setup(self):
self.nie = NIE()
self.spemd = SPEMD(suppress_fastell=True)
self.sis = SIS()
def test_function(self):
y = np.array([1., 2])
x = np.array([0., 0.])
theta_E = 1.
q = 0.9999
s = 0.00001
phi_G = 0
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
values = self.nie.function(x, y, theta_E, e1, e2, s_scale=s)
delta_pot = values[1] - values[0]
values_spemd = self.sis.function(x, y, theta_E)
delta_pot_spemd = values_spemd[1] - values_spemd[0]
npt.assert_almost_equal(delta_pot, delta_pot_spemd, decimal=4)
if bool_test is True:
q = 0.99
s = 0.000001
phi_G = 0
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
values = self.nie.function(x, y, theta_E, e1, e2, s_scale=s)
delta_pot = values[1] - values[0]
gamma = 2.
values_spemd = self.spemd.function(x, y, theta_E, gamma, e1, e2, s_scale=s)
delta_pot_spemd = values_spemd[1] - values_spemd[0]
npt.assert_almost_equal(delta_pot, delta_pot_spemd, decimal=2)
def test_derivatives(self):
x = np.array([1])
y = np.array([2])
theta_E = 1.
q = 0.99999
phi_G = 0
s = 0.0000001
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.nie.derivatives(x, y, theta_E, e1, e2, s_scale=s)
f_x_spemd, f_y_spemd = self.sis.derivatives(x, y, theta_E)
npt.assert_almost_equal(f_x, f_x_spemd, decimal=4)
npt.assert_almost_equal(f_y, f_y_spemd, decimal=4)
if bool_test is True:
q = 0.99
s = 0.000001
phi_G = 0
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.nie.derivatives(x, y, theta_E, e1, e2, s_scale=s)
gamma = 2.
f_x_spemd, f_y_spemd = self.spemd.derivatives(x, y, theta_E, gamma, e1, e2, s_scale=s)
print(f_x/f_x_spemd, 'ratio deflections')
print(1+(1-q)/2)
npt.assert_almost_equal(f_x, f_x_spemd, decimal=2)
npt.assert_almost_equal(f_y, f_y_spemd, decimal=2)
def test_hessian(self):
x = np.array([1])
y = np.array([2])
theta_E = 1.
q = 0.999999
phi_G = 0
s = 0.0000001
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_xx, f_yy, f_xy = self.nie.hessian(x, y, theta_E, e1, e2, s_scale=s)
f_xx_spemd, f_yy_spemd, f_xy_spemd = self.sis.hessian(x, y, theta_E)
npt.assert_almost_equal(f_xx, f_xx_spemd, decimal=4)
npt.assert_almost_equal(f_yy, f_yy_spemd, decimal=4)
npt.assert_almost_equal(f_xy, f_xy_spemd, decimal=4)
def test_convergence2surface_brightness(self):
from lenstronomy.LightModel.Profiles.nie import NIE as NIE_Light
nie_light = NIE_Light()
kwargs = {'e1': 0.3, 'e2': -0.05, 's_scale': 0.5}
x, y = util.make_grid(numPix=10, deltapix=0.1)
f_xx, f_yy, f_xy = self.nie.hessian(x, y, theta_E=1, **kwargs)
kappa = 1/2. * (f_xx + f_yy)
flux = nie_light.function(x, y, amp=1, **kwargs)
npt.assert_almost_equal(kappa/np.sum(kappa), flux/np.sum(flux), decimal=5)
def test_static(self):
x, y = 1., 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_lens = {'theta_E': 1., 's_scale': .1, 'e1': e1, 'e2': e2}
f_ = self.nie.function(x, y, **kwargs_lens)
self.nie.set_static(**kwargs_lens)
f_static = self.nie.function(x, y, **kwargs_lens)
npt.assert_almost_equal(f_, f_static, decimal=8)
self.nie.set_dynamic()
kwargs_lens = {'theta_E': 2., 's_scale': .1, 'e1': e1, 'e2': e2}
f_dyn = self.nie.function(x, y, **kwargs_lens)
assert f_dyn != f_static
class TestSIE(object):
"""
tests the Gaussian methods
"""
def setup(self):
from lenstronomy.LensModel.Profiles.sie import SIE
from lenstronomy.LensModel.Profiles.spemd import SPEMD
from lenstronomy.LensModel.Profiles.nie import NIE
self.sie = SIE(NIE=False)
self.sie_nie = SIE(NIE=True)
self.spemd = SPEMD()
self.nie = NIE()
def test_function(self):
x = np.array([1])
y = np.array([2])
theta_E = 1.
q = 0.9
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
values = self.sie.function(x, y, theta_E, e1, e2)
gamma = 2
values_spemd = self.spemd.function(x, y, theta_E, gamma, e1, e2)
assert values == values_spemd
values = self.sie_nie.function(x, y, theta_E, e1, e2)
s_scale = 0.0000001
values_spemd = self.nie.function(x, y, theta_E, e1, e2, s_scale)
npt.assert_almost_equal(values, values_spemd, decimal=6)
def test_derivatives(self):
x = np.array([1])
y = np.array([2])
theta_E = 1.
q = 0.9
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
values = self.sie.derivatives(x, y, theta_E, e1, e2)
gamma = 2
values_spemd = self.spemd.derivatives(x, y, theta_E, gamma, e1, e2)
assert values == values_spemd
values = self.sie_nie.derivatives(x, y, theta_E, e1, e2)
s_scale = 0.0000001
values_spemd = self.nie.derivatives(x, y, theta_E, e1, e2, s_scale)
npt.assert_almost_equal(values, values_spemd, decimal=6)
def test_hessian(self):
x = np.array([1])
y = np.array([2])
theta_E = 1.
q = 0.9
phi_G = 1.
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
values = self.sie.hessian(x, y, theta_E, e1, e2)
gamma = 2
values_spemd = self.spemd.hessian(x, y, theta_E, gamma, e1, e2)
assert values[0] == values_spemd[0]
values = self.sie_nie.hessian(x, y, theta_E, e1, e2)
s_scale = 0.0000001
values_spemd = self.nie.hessian(x, y, theta_E, e1, e2, s_scale)
npt.assert_almost_equal(values, values_spemd, decimal=5)
class TestSPEMD(object):
"""
tests the Gaussian methods
"""
def setup(self):
from lenstronomy.LensModel.Profiles.spemd import SPEMD
self.SPEMD = SPEMD(suppress_fastell=True)
from lenstronomy.LensModel.Profiles.nie import NIE
self.NIE = NIE()
def test_function(self):
phi_E = 1.
gamma = 2.
q = 0.999
phi_G = 1.
s_scale = 0.1
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
x = np.array([1., 2])
y = np.array([2, 0])
values = self.SPEMD.function(x, y, phi_E, gamma, e1, e2, s_scale)
if fastell4py_bool:
values_nie = self.NIE.function(x, y, phi_E, e1, e2, s_scale)
delta_f = values[0] - values[1]
delta_f_nie = values_nie[0] - values_nie[1]
npt.assert_almost_equal(delta_f, delta_f_nie, decimal=5)
else:
npt.assert_almost_equal(values, 0, decimal=5)
def test_derivatives(self):
x = np.array([1])
y = np.array([2])
phi_E = 1.
gamma = 2.
q = 1.
phi_G = 1.
s_scale = 0.1
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.SPEMD.derivatives(x, y, phi_E, gamma, e1, e2, s_scale)
if fastell4py_bool:
f_x_nie, f_y_nie = self.NIE.derivatives(x, y, phi_E, e1, e2,
s_scale)
npt.assert_almost_equal(f_x, f_x_nie, decimal=4)
npt.assert_almost_equal(f_y, f_y_nie, decimal=4)
else:
npt.assert_almost_equal(f_x, 0, decimal=7)
npt.assert_almost_equal(f_y, 0, decimal=7)
q = 0.7
phi_G = 1.
s_scale = 0.001
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.SPEMD.derivatives(x, y, phi_E, gamma, e1, e2, s_scale)
if fastell4py_bool:
f_x_nie, f_y_nie = self.NIE.derivatives(x, y, phi_E, e1, e2,
s_scale)
npt.assert_almost_equal(f_x, f_x_nie, decimal=4)
npt.assert_almost_equal(f_y, f_y_nie, decimal=4)
else:
npt.assert_almost_equal(f_x, 0, decimal=7)
npt.assert_almost_equal(f_y, 0, decimal=7)
def test_hessian(self):
x = np.array([1.])
y = np.array([2.])
phi_E = 1.
gamma = 2.
q = 0.9
phi_G = 1.
s_scale = 0.001
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_xx, f_xy, f_yx, f_yy = self.SPEMD.hessian(x, y, phi_E, gamma, e1, e2,
s_scale)
if fastell4py_bool:
f_xx_nie, f_xy_nie, f_yx_nie, f_yy_nie = self.NIE.hessian(
x, y, phi_E, e1, e2, s_scale)
npt.assert_almost_equal(f_xx, f_xx_nie, decimal=4)
npt.assert_almost_equal(f_yy, f_yy_nie, decimal=4)
npt.assert_almost_equal(f_xy, f_xy_nie, decimal=4)
npt.assert_almost_equal(f_yx, f_yx_nie, decimal=4)
else:
npt.assert_almost_equal(f_xx, 0, decimal=7)
npt.assert_almost_equal(f_yy, 0, decimal=7)
npt.assert_almost_equal(f_xy, 0, decimal=7)
npt.assert_almost_equal(f_xy, f_yx, decimal=8)
def test_bounds(self):
compute_bool = self.SPEMD._parameter_constraints(q_fastell=-1,
gam=-1,
s2=-1,
q=-1)
assert compute_bool is False
def test_is_not_empty(self):
func = self.SPEMD.is_not_empty
assert func(0.1, 0.2)
assert func([0.1], [0.2])
assert func((0.1, 0.3), (0.2, 0.4))
assert func(np.array([0.1]), np.array([0.2]))
assert not func([], [])
assert not func(np.array([]), np.array([]))
def setup(self):
from lenstronomy.LensModel.Profiles.spemd_smooth import SPEMD_SMOOTH
self.SPEMD_SMOOT = SPEMD_SMOOTH()
from lenstronomy.LensModel.Profiles.nie import NIE
self.NIE = NIE()
def _import_class(lens_type, custom_class, z_lens=None, z_source=None):
"""
:param lens_type: string, lens model type
:param custom_class: custom class
:param z_lens: lens redshift # currently only used in NFW_MC model as this is redshift dependent
:param z_source: source redshift # currently only used in NFW_MC model as this is redshift dependent
:return: class instance of the lens model type
"""
if lens_type == 'SHIFT':
from lenstronomy.LensModel.Profiles.alpha_shift import Shift
return Shift()
elif lens_type == 'SHEAR':
from lenstronomy.LensModel.Profiles.shear import Shear
return Shear()
elif lens_type == 'SHEAR_GAMMA_PSI':
from lenstronomy.LensModel.Profiles.shear import ShearGammaPsi
return ShearGammaPsi()
elif lens_type == 'CONVERGENCE':
from lenstronomy.LensModel.Profiles.convergence import Convergence
return Convergence()
elif lens_type == 'FLEXION':
from lenstronomy.LensModel.Profiles.flexion import Flexion
return Flexion()
elif lens_type == 'FLEXIONFG':
from lenstronomy.LensModel.Profiles.flexionfg import Flexionfg
return Flexionfg()
elif lens_type == 'POINT_MASS':
from lenstronomy.LensModel.Profiles.point_mass import PointMass
return PointMass()
elif lens_type == 'SIS':
from lenstronomy.LensModel.Profiles.sis import SIS
return SIS()
elif lens_type == 'SIS_TRUNCATED':
from lenstronomy.LensModel.Profiles.sis_truncate import SIS_truncate
return SIS_truncate()
elif lens_type == 'SIE':
from lenstronomy.LensModel.Profiles.sie import SIE
return SIE()
elif lens_type == 'SPP':
from lenstronomy.LensModel.Profiles.spp import SPP
return SPP()
elif lens_type == 'NIE':
from lenstronomy.LensModel.Profiles.nie import NIE
return NIE()
elif lens_type == 'NIE_SIMPLE':
from lenstronomy.LensModel.Profiles.nie import NIEMajorAxis
return NIEMajorAxis()
elif lens_type == 'CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import Chameleon
return Chameleon()
elif lens_type == 'DOUBLE_CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import DoubleChameleon
return DoubleChameleon()
elif lens_type == 'TRIPLE_CHAMELEON':
from lenstronomy.LensModel.Profiles.chameleon import TripleChameleon
return TripleChameleon()
elif lens_type == 'SPEP':
from lenstronomy.LensModel.Profiles.spep import SPEP
return SPEP()
elif lens_type == 'SPEMD':
from lenstronomy.LensModel.Profiles.spemd import SPEMD
return SPEMD()
elif lens_type == 'SPEMD_SMOOTH':
from lenstronomy.LensModel.Profiles.spemd_smooth import SPEMD_SMOOTH
return SPEMD_SMOOTH()
elif lens_type == 'NFW':
from lenstronomy.LensModel.Profiles.nfw import NFW
return NFW()
elif lens_type == 'NFW_ELLIPSE':
from lenstronomy.LensModel.Profiles.nfw_ellipse import NFW_ELLIPSE
return NFW_ELLIPSE()
elif lens_type == 'NFW_ELLIPSE_GAUSS_DEC':
from lenstronomy.LensModel.Profiles.gauss_decomposition import NFWEllipseGaussDec
return NFWEllipseGaussDec()
elif lens_type == 'TNFW':
from lenstronomy.LensModel.Profiles.tnfw import TNFW
return TNFW()
elif lens_type == 'CNFW':
from lenstronomy.LensModel.Profiles.cnfw import CNFW
return CNFW()
elif lens_type == 'CNFW_ELLIPSE':
from lenstronomy.LensModel.Profiles.cnfw_ellipse import CNFW_ELLIPSE
return CNFW_ELLIPSE()
elif lens_type == 'CTNFW_GAUSS_DEC':
from lenstronomy.LensModel.Profiles.gauss_decomposition import CTNFWGaussDec
return CTNFWGaussDec()
elif lens_type == 'NFW_MC':
from lenstronomy.LensModel.Profiles.nfw_mass_concentration import NFWMC
return NFWMC(z_lens=z_lens, z_source=z_source)
elif lens_type == 'SERSIC':
from lenstronomy.LensModel.Profiles.sersic import Sersic
return Sersic()
elif lens_type == 'SERSIC_ELLIPSE_POTENTIAL':
from lenstronomy.LensModel.Profiles.sersic_ellipse_potential import SersicEllipse
return SersicEllipse()
elif lens_type == 'SERSIC_ELLIPSE_KAPPA':
from lenstronomy.LensModel.Profiles.sersic_ellipse_kappa import SersicEllipseKappa
return SersicEllipseKappa()
elif lens_type == 'SERSIC_ELLIPSE_GAUSS_DEC':
from lenstronomy.LensModel.Profiles.gauss_decomposition \
import SersicEllipseGaussDec
return SersicEllipseGaussDec()
elif lens_type == 'PJAFFE':
from lenstronomy.LensModel.Profiles.p_jaffe import PJaffe
return PJaffe()
elif lens_type == 'PJAFFE_ELLIPSE':
from lenstronomy.LensModel.Profiles.p_jaffe_ellipse import PJaffe_Ellipse
return PJaffe_Ellipse()
elif lens_type == 'HERNQUIST':
from lenstronomy.LensModel.Profiles.hernquist import Hernquist
return Hernquist()
elif lens_type == 'HERNQUIST_ELLIPSE':
from lenstronomy.LensModel.Profiles.hernquist_ellipse import Hernquist_Ellipse
return Hernquist_Ellipse()
elif lens_type == 'GAUSSIAN':
from lenstronomy.LensModel.Profiles.gaussian_potential import Gaussian
return Gaussian()
elif lens_type == 'GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.gaussian_kappa import GaussianKappa
return GaussianKappa()
elif lens_type == 'GAUSSIAN_ELLIPSE_KAPPA':
from lenstronomy.LensModel.Profiles.gaussian_ellipse_kappa import GaussianEllipseKappa
return GaussianEllipseKappa()
elif lens_type == 'GAUSSIAN_ELLIPSE_POTENTIAL':
from lenstronomy.LensModel.Profiles.gaussian_ellipse_potential import GaussianEllipsePotential
return GaussianEllipsePotential()
elif lens_type == 'MULTI_GAUSSIAN_KAPPA':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappa
return MultiGaussianKappa()
elif lens_type == 'MULTI_GAUSSIAN_KAPPA_ELLIPSE':
from lenstronomy.LensModel.Profiles.multi_gaussian_kappa import MultiGaussianKappaEllipse
return MultiGaussianKappaEllipse()
elif lens_type == 'INTERPOL':
from lenstronomy.LensModel.Profiles.interpol import Interpol
return Interpol()
elif lens_type == 'INTERPOL_SCALED':
from lenstronomy.LensModel.Profiles.interpol import InterpolScaled
return InterpolScaled()
elif lens_type == 'SHAPELETS_POLAR':
from lenstronomy.LensModel.Profiles.shapelet_pot_polar import PolarShapelets
return PolarShapelets()
elif lens_type == 'SHAPELETS_CART':
from lenstronomy.LensModel.Profiles.shapelet_pot_cartesian import CartShapelets
return CartShapelets()
elif lens_type == 'DIPOLE':
from lenstronomy.LensModel.Profiles.dipole import Dipole
return Dipole()
elif lens_type == 'CURVED_ARC':
from lenstronomy.LensModel.Profiles.curved_arc import CurvedArc
return CurvedArc()
elif lens_type == 'ARC_PERT':
from lenstronomy.LensModel.Profiles.arc_perturbations import ArcPerturbations
return ArcPerturbations()
elif lens_type == 'coreBURKERT':
from lenstronomy.LensModel.Profiles.coreBurkert import CoreBurkert
return CoreBurkert()
elif lens_type == 'CORED_DENSITY':
from lenstronomy.LensModel.Profiles.cored_density import CoredDensity
return CoredDensity()
elif lens_type == 'CORED_DENSITY_2':
from lenstronomy.LensModel.Profiles.cored_density_2 import CoredDensity2
return CoredDensity2()
elif lens_type == 'CORED_DENSITY_MST':
from lenstronomy.LensModel.Profiles.cored_density_mst import CoredDensityMST
return CoredDensityMST(profile_type='CORED_DENSITY')
elif lens_type == 'CORED_DENSITY_2_MST':
from lenstronomy.LensModel.Profiles.cored_density_mst import CoredDensityMST
return CoredDensityMST(profile_type='CORED_DENSITY_2')
elif lens_type == 'NumericalAlpha':
from lenstronomy.LensModel.Profiles.numerical_deflections import NumericalAlpha
return NumericalAlpha(custom_class)
else:
raise ValueError('%s is not a valid lens model' % lens_type)
class TestNIE(object):
"""
tests the Gaussian methods
"""
def setup(self):
from lenstronomy.LensModel.Profiles.nie import NIE
from lenstronomy.LensModel.Profiles.spemd_smooth import SPEMD_SMOOTH
from lenstronomy.LensModel.Profiles.sis import SIS
self.nie = NIE()
self.spemd = SPEMD_SMOOTH()
self.sis = SIS()
def test_function(self):
y = np.array([1., 2])
x = np.array([0., 0.])
theta_E = 1.
q = 0.9999
s = 0.00001
phi_G = 0
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
values = self.nie.function(x, y, theta_E, e1, e2, s_scale=s)
delta_pot = values[1] - values[0]
values_spemd = self.sis.function(x, y, theta_E)
delta_pot_spemd = values_spemd[1] - values_spemd[0]
npt.assert_almost_equal(delta_pot, delta_pot_spemd, decimal=4)
if bool_test is True:
q = 0.99
s = 0.000001
phi_G = 0
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
values = self.nie.function(x, y, theta_E, e1, e2, s_scale=s)
delta_pot = values[1] - values[0]
gamma = 2.
values_spemd = self.spemd.function(x,
y,
theta_E,
gamma,
e1,
e2,
s_scale=s)
delta_pot_spemd = values_spemd[1] - values_spemd[0]
npt.assert_almost_equal(delta_pot, delta_pot_spemd, decimal=2)
def test_derivatives(self):
x = np.array([1])
y = np.array([2])
theta_E = 1.
q = 0.99999
phi_G = 0
s = 0.0000001
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.nie.derivatives(x, y, theta_E, e1, e2, s_scale=s)
f_x_spemd, f_y_spemd = self.sis.derivatives(x, y, theta_E)
npt.assert_almost_equal(f_x, f_x_spemd, decimal=4)
npt.assert_almost_equal(f_y, f_y_spemd, decimal=4)
if bool_test is True:
q = 0.99
s = 0.000001
phi_G = 0
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_x, f_y = self.nie.derivatives(x, y, theta_E, e1, e2, s_scale=s)
gamma = 2.
f_x_spemd, f_y_spemd = self.spemd.derivatives(x,
y,
theta_E,
gamma,
e1,
e2,
s_scale=s)
print(f_x / f_x_spemd, 'ratio deflections')
print(1 + (1 - q) / 2)
npt.assert_almost_equal(f_x, f_x_spemd, decimal=2)
npt.assert_almost_equal(f_y, f_y_spemd, decimal=2)
def test_hessian(self):
x = np.array([1])
y = np.array([2])
theta_E = 1.
q = 0.999999
phi_G = 0
s = 0.0000001
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
f_xx, f_yy, f_xy = self.nie.hessian(x, y, theta_E, e1, e2, s_scale=s)
f_xx_spemd, f_yy_spemd, f_xy_spemd = self.sis.hessian(x, y, theta_E)
npt.assert_almost_equal(f_xx, f_xx_spemd, decimal=4)
npt.assert_almost_equal(f_yy, f_yy_spemd, decimal=4)
npt.assert_almost_equal(f_xy, f_xy_spemd, decimal=4)
class TestChameleon(object):
"""
class to test the Moffat profile
"""
def setup(self):
self.chameleon = Chameleon()
self.nie = NIE()
def test_theta_E_convert(self):
w_c, w_t = 2, 1
theta_E_convert, w_c, w_t = self.chameleon._theta_E_convert(theta_E=1,
w_c=w_c,
w_t=w_t)
assert w_c == 1
assert w_t == 2
def test_function(self):
"""
:return:
"""
x = np.linspace(0.1, 10, 10)
w_c, w_t = 0.5, 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_light = {
'theta_E': 1.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
theta_E_convert, w_c, w_t = self.chameleon._theta_E_convert(theta_E=1,
w_c=0.5,
w_t=1.)
s_scale_1 = np.sqrt(4 * w_c**2 / (1. + q)**2)
s_scale_2 = np.sqrt(4 * w_t**2 / (1. + q)**2)
kwargs_1 = {
'theta_E': theta_E_convert,
's_scale': s_scale_1,
'e1': e1,
'e2': e2
}
kwargs_2 = {
'theta_E': theta_E_convert,
's_scale': s_scale_2,
'e1': e1,
'e2': e2
}
f_ = self.chameleon.function(x=x, y=1., **kwargs_light)
f_1 = self.nie.function(x=x, y=1., **kwargs_1)
f_2 = self.nie.function(x=x, y=1., **kwargs_2)
npt.assert_almost_equal(f_, (f_1 - f_2), decimal=5)
def test_derivatives(self):
"""
:return:
"""
x = np.linspace(0.1, 10, 10)
w_c, w_t = 0.5, 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_light = {
'theta_E': 1.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
theta_E_convert, w_c, w_t = self.chameleon._theta_E_convert(theta_E=1,
w_c=0.5,
w_t=1.)
s_scale_1 = np.sqrt(4 * w_c**2 / (1. + q)**2)
s_scale_2 = np.sqrt(4 * w_t**2 / (1. + q)**2)
kwargs_1 = {
'theta_E': theta_E_convert,
's_scale': s_scale_1,
'e1': e1,
'e2': e2
}
kwargs_2 = {
'theta_E': theta_E_convert,
's_scale': s_scale_2,
'e1': e1,
'e2': e2
}
f_x, f_y = self.chameleon.derivatives(x=x, y=1., **kwargs_light)
f_x_1, f_y_1 = self.nie.derivatives(x=x, y=1., **kwargs_1)
f_x_2, f_y_2 = self.nie.derivatives(x=x, y=1., **kwargs_2)
npt.assert_almost_equal(f_x, (f_x_1 - f_x_2), decimal=5)
npt.assert_almost_equal(f_y, (f_y_1 - f_y_2), decimal=5)
f_x, f_y = self.chameleon.derivatives(x=1, y=0., **kwargs_light)
npt.assert_almost_equal(f_x, 1, decimal=1)
def test_hessian(self):
"""
:return:
"""
x = np.linspace(0.1, 10, 10)
w_c, w_t = 0.5, 1.
phi_G, q = 0.3, 0.8
e1, e2 = param_util.phi_q2_ellipticity(phi_G, q)
kwargs_light = {
'theta_E': 1.,
'w_c': .5,
'w_t': 1.,
'e1': e1,
'e2': e2
}
theta_E_convert, w_c, w_t = self.chameleon._theta_E_convert(theta_E=1,
w_c=0.5,
w_t=1.)
s_scale_1 = np.sqrt(4 * w_c**2 / (1. + q)**2)
s_scale_2 = np.sqrt(4 * w_t**2 / (1. + q)**2)
kwargs_1 = {
'theta_E': theta_E_convert,
's_scale': s_scale_1,
'e1': e1,
'e2': e2
}
kwargs_2 = {
'theta_E': theta_E_convert,
's_scale': s_scale_2,
'e1': e1,
'e2': e2
}
f_xx, f_yy, f_xy = self.chameleon.hessian(x=x, y=1., **kwargs_light)
f_xx_1, f_yy_1, f_xy_1 = self.nie.hessian(x=x, y=1., **kwargs_1)
f_xx_2, f_yy_2, f_xy_2 = self.nie.hessian(x=x, y=1., **kwargs_2)
npt.assert_almost_equal(f_xx, (f_xx_1 - f_xx_2), decimal=5)
npt.assert_almost_equal(f_yy, (f_yy_1 - f_yy_2), decimal=5)
npt.assert_almost_equal(f_xy, (f_xy_1 - f_xy_2), decimal=5)
class Chameleon(object):
"""
class of the Chameleon model (See Suyu+2014) an elliptical truncated double isothermal profile
"""
param_names = ['theta_E', 'w_c', 'w_t', 'e1', 'e2', 'center_x', 'center_y']
lower_limit_default = {
'theta_E': 0,
'w_c': 0,
'w_t': 0,
'e1': -0.8,
'e2': -0.8,
'center_x': -100,
'center_y': -100
}
upper_limit_default = {
'theta_E': 100,
'w_c': 100,
'w_t': 100,
'e1': 0.8,
'e2': 0.8,
'center_x': 100,
'center_y': 100
}
def __init__(self):
self.nie = NIE()
def function(self,
x,
y,
theta_E,
w_c,
w_t,
e1,
e2,
center_x=0,
center_y=0):
"""
:param x: ra-coordinate
:param y: dec-coordinate
:param amp: amplitude of first power-law flux
:param flux_ratio: ratio of amplitudes of first to second power-law profile
:param gamma1: power-law slope
:param gamma2: power-law slope
:param e1: ellipticity parameter
:param e2: ellipticity parameter
:param center_x: center
:param center_y: center
:return: flux of chameleon profile
"""
theta_E_conv, w_c, w_t = self._theta_E_convert(theta_E, w_c, w_t)
#if not w_t > w_c:
# w_t, w_c = w_c, w_t
phi_G, q = param_util.ellipticity2phi_q(e1, e2)
s_scale_1 = np.sqrt(4 * w_c**2 / (1. + q)**2)
s_scale_2 = np.sqrt(4 * w_t**2 / (1. + q)**2)
f_1 = self.nie.function(x, y, theta_E_conv, e1, e2, s_scale_1,
center_x, center_y)
f_2 = self.nie.function(x, y, theta_E_conv, e1, e2, s_scale_2,
center_x, center_y)
f_ = f_1 - f_2
return f_
def derivatives(self,
x,
y,
theta_E,
w_c,
w_t,
e1,
e2,
center_x=0,
center_y=0):
"""
:param x: ra-coordinate
:param y: dec-coordinate
:param amp: amplitude of first power-law flux
:param flux_ratio: ratio of amplitudes of first to second power-law profile
:param gamma1: power-law slope
:param gamma2: power-law slope
:param e1: ellipticity parameter
:param e2: ellipticity parameter
:param center_x: center
:param center_y: center
:return: flux of chameleon profile
"""
theta_E_conv, w_c, w_t = self._theta_E_convert(theta_E, w_c, w_t)
#if not w_t > w_c:
# w_t, w_c = w_c, w_t
phi_G, q = param_util.ellipticity2phi_q(e1, e2)
s_scale_1 = np.sqrt(4 * w_c**2 / (1. + q)**2)
s_scale_2 = np.sqrt(4 * w_t**2 / (1. + q)**2)
f_x_1, f_y_1 = self.nie.derivatives(x, y, theta_E_conv, e1, e2,
s_scale_1, center_x, center_y)
f_x_2, f_y_2 = self.nie.derivatives(x, y, theta_E_conv, e1, e2,
s_scale_2, center_x, center_y)
f_x = f_x_1 - f_x_2
f_y = f_y_1 - f_y_2
return f_x, f_y
def hessian(self, x, y, theta_E, w_c, w_t, e1, e2, center_x=0, center_y=0):
"""
:param x: ra-coordinate
:param y: dec-coordinate
:param theta_E: amplitude of first power-law flux
:param flux_ratio: ratio of amplitudes of first to second power-law profile
:param gamma1: power-law slope
:param gamma2: power-law slope
:param e1: ellipticity parameter
:param e2: ellipticity parameter
:param center_x: center
:param center_y: center
:return: flux of chameleon profile
"""
theta_E_conv, w_c, w_t = self._theta_E_convert(theta_E, w_c, w_t)
#if not w_t > w_c:
# w_t, w_c = w_c, w_t
phi_G, q = param_util.ellipticity2phi_q(e1, e2)
s_scale_1 = np.sqrt(4 * w_c**2 / (1. + q)**2)
s_scale_2 = np.sqrt(4 * w_t**2 / (1. + q)**2)
f_xx_1, f_yy_1, f_xy_1 = self.nie.hessian(x, y, theta_E_conv, e1, e2,
s_scale_1, center_x,
center_y)
f_xx_2, f_yy_2, f_xy_2 = self.nie.hessian(x, y, theta_E_conv, e1, e2,
s_scale_2, center_x,
center_y)
f_xx = f_xx_1 - f_xx_2
f_yy = f_yy_1 - f_yy_2
f_xy = f_xy_1 - f_xy_2
return f_xx, f_yy, f_xy
def _theta_E_convert(self, theta_E, w_c, w_t):
"""
convert the parameter theta_E (deflection angle one arcsecond from the center) into the
"Einstein radius" scale parameter of the two NIE profiles
:param theta_E:
:param w_c:
:param w_t:
:return:
"""
if not w_t > w_c:
w_t, w_c = w_c, w_t
s_scale_1 = w_c
s_scale_2 = w_t
f_x_1, f_y_1 = self.nie.derivatives(1,
0,
theta_E=1,
e1=0,
e2=0,
s_scale=s_scale_1)
f_x_2, f_y_2 = self.nie.derivatives(1,
0,
theta_E=1,
e1=0,
e2=0,
s_scale=s_scale_2)
f_x = f_x_1 - f_x_2
theta_E_convert = theta_E / f_x
return theta_E_convert, w_c, w_t
