コード例 #1
0
def psf_configure_simple(psf_type="GAUSSIAN",
                         fwhm=1,
                         kernelsize=11,
                         deltaPix=1,
                         truncate=6,
                         kernel=None):
    """
    this routine generates keyword arguments to initialize a PSF() class in lenstronomy. Have a look at the PSF class
    documentation to see the full possibilities.

    :param psf_type: string, type of PSF model
    :param fwhm: Full width at half maximum of PSF (if GAUSSIAN psf)
    :param kernelsize: size in pixel of kernel (use odd numbers), only applicable for PIXEL kernels
    :param deltaPix: pixel size in angular units (only needed for GAUSSIAN kernel
    :param truncate: how many sigmas out is the truncation happening
    :param kernel: 2d numpy arra centered PSF (odd number per axis)
    :return: keyword arguments
    """

    if psf_type == 'GAUSSIAN':
        sigma = util.fwhm2sigma(fwhm)
        sigma_axis = sigma
        gaussian = Gaussian()
        x_grid, y_grid = util.make_grid(kernelsize, deltaPix)
        kernel_large = gaussian.function(x_grid,
                                         y_grid,
                                         amp=1.,
                                         sigma_x=sigma_axis,
                                         sigma_y=sigma_axis,
                                         center_x=0,
                                         center_y=0)
        kernel_large /= np.sum(kernel_large)
        kernel_large = util.array2image(kernel_large)
        kernel_pixel = kernel_util.pixel_kernel(kernel_large)
        kwargs_psf = {
            'psf_type': psf_type,
            'fwhm': fwhm,
            'truncation': truncate * fwhm,
            'kernel_point_source': kernel_large,
            'kernel_pixel': kernel_pixel,
            'pixel_size': deltaPix
        }
    elif psf_type == 'PIXEL':
        kernel_large = copy.deepcopy(kernel)
        kernel_large = kernel_util.cut_psf(kernel_large, psf_size=kernelsize)
        kwargs_psf = {'psf_type': "PIXEL", 'kernel_point_source': kernel_large}
    elif psf_type == 'NONE':
        kwargs_psf = {'psf_type': 'NONE'}
    else:
        raise ValueError("psf type %s not supported!" % psf_type)
    return kwargs_psf
コード例 #2
0
    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)
コード例 #3
0
    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
コード例 #4
0
ファイル: simulations.py プロジェクト: guoxiaowhu/lenstronomy
class Simulation(object):
    """
    simulation class that querries the major class of lenstronomy
    """
    def __init__(self):
        self.gaussian = Gaussian()

    def data_configure(self, numPix, deltaPix, exposure_time=1, sigma_bkg=1):
        """
        configures the data keyword arguments with a coordinate grid centered at zero.

        :param numPix: number of pixel (numPix x numPix)
        :param deltaPix: pixel size
        :param exposure_time: exposure time
        :param sigma_bkg: background noise (Gaussian sigma)
        :return:
        """
        mean = 0.  # background mean flux (default zero)
        # 1d list of coordinates (x,y) of a numPix x numPix square grid, centered to zero
        x_grid, y_grid, ra_at_xy_0, dec_at_xy_0, x_at_radec_0, y_at_radec_0, Mpix2coord, Mcoord2pix = util.make_grid_with_coordtransform(numPix=numPix, deltapix=deltaPix, subgrid_res=1)
        # mask (1= model this pixel, 0= leave blanck)
        exposure_map = np.ones((numPix, numPix)) * exposure_time  # individual exposure time/weight per pixel

        kwargs_data = {
            'background_rms': sigma_bkg,
            'exposure_map': exposure_map
            , 'ra_at_xy_0': ra_at_xy_0, 'dec_at_xy_0': dec_at_xy_0, 'transform_pix2angle': Mpix2coord
            , 'image_data': np.zeros((numPix, numPix))
            }
        return kwargs_data

    def psf_configure(self, psf_type="GAUSSIAN", fwhm=1, kernelsize=11, deltaPix=1, truncate=6, kernel=None):
        """

        :param psf_type:
        :param fwhm:
        :param pixel_grid:
        :return:
        """
        # psf_type: 'NONE', 'gaussian', 'pixel'
        # 'pixel': kernel, kernel_large
        # 'gaussian': 'sigma', 'truncate'
        if psf_type == 'GAUSSIAN':
            sigma = util.fwhm2sigma(fwhm)
            sigma_axis = sigma
            x_grid, y_grid = util.make_grid(kernelsize, deltaPix)
            kernel_large = self.gaussian.function(x_grid, y_grid, amp=1., sigma_x=sigma_axis, sigma_y=sigma_axis, center_x=0, center_y=0)
            kernel_large /= np.sum(kernel_large)
            kernel_large = util.array2image(kernel_large)
            kernel_pixel = kernel_util.pixel_kernel(kernel_large)
            kwargs_psf = {'psf_type': psf_type, 'fwhm': fwhm, 'truncation': truncate*fwhm, 'kernel_point_source': kernel_large, 'kernel_pixel': kernel_pixel, 'pixel_size': deltaPix}
        elif psf_type == 'PIXEL':
            kernel_large = copy.deepcopy(kernel)
            kernel_large = kernel_util.cut_psf(kernel_large, psf_size=kernelsize)
            kernel_small = copy.deepcopy(kernel)
            kernel_small = kernel_util.cut_psf(kernel_small, psf_size=kernelsize)
            #kwargs_psf = {'psf_type': "PIXEL", 'kernel_pixel': kernel_small, 'kernel_point_source': kernel_large}
            kwargs_psf = {'psf_type': "PIXEL", 'kernel_point_source': kernel_large}
        elif psf_type == 'NONE':
            kwargs_psf = {'psf_type': 'NONE'}
        else:
            raise ValueError("psf type %s not supported!" % psf_type)
        return kwargs_psf

    def normalize_flux(self, kwargs_options, kwargs_source, kwargs_lens_light, kwargs_ps, norm_factor_source=1, norm_factor_lens_light=1, norm_factor_point_source=1.):
        """
        multiplies the surface brightness amplitudes with a norm_factor
        aim: mimic different telescopes photon collection area or colours for different imaging bands
        :param kwargs_source:
        :param kwargs_lens_light:
        :param norm_factor:
        :return:
        """
        lensLightModel = LightModel(kwargs_options.get('lens_light_model_list', []))
        sourceModel = LightModel(kwargs_options.get('source_light_model_list', []))
        lensModel = LensModel(lens_model_list=kwargs_options.get('lens_model_list', []))
        pointSource = PointSource(point_source_type_list=kwargs_options.get('point_source_list', []),
                                          lensModel=lensModel, fixed_magnification_list=kwargs_options.get('fixed_magnification_list', [False]),
                                       additional_images_list=kwargs_options.get('additional_images_list', [False]))
        kwargs_source_updated = copy.deepcopy(kwargs_source)
        kwargs_lens_light_updated = copy.deepcopy(kwargs_lens_light)
        kwargs_ps_updated = copy.deepcopy(kwargs_ps)
        kwargs_source_updated = sourceModel.re_normalize_flux(kwargs_source_updated, norm_factor_source)
        kwargs_lens_light_updated = lensLightModel.re_normalize_flux(kwargs_lens_light_updated, norm_factor_lens_light)
        kwargs_ps_updated = pointSource.re_normalize_flux(kwargs_ps_updated, norm_factor_point_source)
        return kwargs_source_updated, kwargs_lens_light_updated, kwargs_ps_updated

    def normalize_flux_source(self, kwargs_options, kwargs_source, norm_factor_source):
        """
        normalized the flux of the source
        :param kwargs_options:
        :param kwargs_source:
        :param norm_factor_source:
        :return:
        """
        kwargs_source_updated = copy.deepcopy(kwargs_source)
        sourceModel = LightModel(kwargs_options.get('source_light_model_list', []))
        kwargs_source_updated = sourceModel.re_normalize_flux(kwargs_source_updated, norm_factor_source)
        return kwargs_source_updated

    def simulate(self, image_model_class, kwargs_lens=None, kwargs_source=None, kwargs_lens_light=None, kwargs_ps=None,
                 no_noise=False, source_add=True, lens_light_add=True, point_source_add=True):
        """
        simulate image
        :param kwargs_options:
        :param kwargs_data:
        :param kwargs_psf:
        :param kwargs_lens:
        :param kwargs_source:
        :param kwargs_lens_light:
        :param kwargs_ps:
        :param no_noise:
        :return:
        """
        image = image_model_class.image(kwargs_lens, kwargs_source, kwargs_lens_light, kwargs_ps, source_add=source_add, lens_light_add=lens_light_add, point_source_add=point_source_add)
        # add noise
        if no_noise:
            return image
        else:
            poisson = image_util.add_poisson(image, exp_time=image_model_class.Data.exposure_map)
            bkg = image_util.add_background(image, sigma_bkd=image_model_class.Data.background_rms)
            return image + bkg + poisson

    def source_plane(self, kwargs_options, kwargs_source, numPix, deltaPix):
        """
        source plane simulation
        :param kwargs_options:
        :param kwargs_source:
        :param numPix:
        :param deltaPix:
        :return:
        """
        x, y = util.make_grid(numPix, deltaPix)
        sourceModel = LightModel(kwargs_options.get('source_light_model_list', []))
        image1d = sourceModel.surface_brightness(x, y, kwargs_source)
        image2d = util.array2image(image1d)
        return image2d
コード例 #5
0
ファイル: simulations.py プロジェクト: guoxiaowhu/lenstronomy
 def __init__(self):
     self.gaussian = Gaussian()
コード例 #6
0
class TestGaussianKappa(object):
    """
    test the Gaussian with Gaussian kappa
    """
    def setup(self):
        self.gaussian_kappa = GaussianKappa()
        self.gaussian = Gaussian()

    def test_derivatives(self):
        x = np.linspace(0, 5, 10)
        y = np.linspace(0, 5, 10)
        amp = 1. * 2 * np.pi
        center_x = 0.
        center_y = 0.
        sigma = 1.
        f_x, f_y = self.gaussian_kappa.derivatives(x, y, amp, sigma, center_x,
                                                   center_y)
        npt.assert_almost_equal(f_x[2], 0.63813558702212059, decimal=8)
        npt.assert_almost_equal(f_y[2], 0.63813558702212059, decimal=8)

    def test_hessian(self):
        x = np.linspace(0, 5, 10)
        y = np.linspace(0, 5, 10)
        amp = 1. * 2 * np.pi
        center_x = 0.
        center_y = 0.
        sigma = 1.

        f_xx, f_yy, f_xy = self.gaussian_kappa.hessian(x, y, amp, sigma,
                                                       center_x, center_y)
        kappa = 1. / 2 * (f_xx + f_yy)
        kappa_true = self.gaussian.function(x, y, amp, sigma, sigma, center_x,
                                            center_y)
        print(kappa_true)
        print(kappa)
        npt.assert_almost_equal(kappa[0], kappa_true[0], decimal=5)
        npt.assert_almost_equal(kappa[1], kappa_true[1], decimal=5)

    def test_density_2d(self):
        x = np.linspace(0, 5, 10)
        y = np.linspace(0, 5, 10)
        amp = 1. * 2 * np.pi
        center_x = 0.
        center_y = 0.
        sigma = 1.
        f_xx, f_yy, f_xy = self.gaussian_kappa.hessian(x, y, amp, sigma,
                                                       center_x, center_y)
        kappa = 1. / 2 * (f_xx + f_yy)
        amp_3d = self.gaussian_kappa._amp2d_to_3d(amp, sigma, sigma)
        density_2d = self.gaussian_kappa.density_2d(x, y, amp_3d, sigma,
                                                    center_x, center_y)
        npt.assert_almost_equal(kappa[1], density_2d[1], decimal=5)
        npt.assert_almost_equal(kappa[2], density_2d[2], decimal=5)

    def test_3d_2d_convention(self):
        x = np.linspace(0, 5, 10)
        y = np.linspace(0, 5, 10)
        amp = 1. * 2 * np.pi
        center_x = 0.
        center_y = 0.
        sigma = 1.
        amp_3d = self.gaussian_kappa._amp2d_to_3d(amp, sigma, sigma)
        density_2d_gauss = self.gaussian_kappa.density_2d(
            x, y, amp_3d, sigma, center_x, center_y)
        density_2d = self.gaussian.function(x, y, amp, sigma, sigma, center_x,
                                            center_y)
        npt.assert_almost_equal(density_2d_gauss[1], density_2d[1], decimal=5)
コード例 #7
0
 def setup(self):
     self.gaussian_kappa = GaussianKappa()
     self.gaussian = Gaussian()
コード例 #8
0
class TestGaussian(object):
    """
    tests the Gaussian methods
    """
    def setup(self):
        self.Gaussian = Gaussian()

    def test_function(self):
        x = 1
        y = 2
        amp = 1. * 2 * np.pi
        center_x = 1.
        center_y = 1.
        sigma_x = 1.
        sigma_y = 1.
        values = self.Gaussian.function(x, y, amp, center_x, center_y, sigma_x,
                                        sigma_y)
        assert values == np.exp(-1. / 2)
        x = np.array([2, 3, 4])
        y = np.array([1, 1, 1])
        values = self.Gaussian.function(x, y, amp, center_x, center_y, sigma_x,
                                        sigma_y)
        assert values[0] == np.exp(-1. / 2)
        assert values[1] == np.exp(-2.**2 / 2)
        assert values[2] == np.exp(-3.**2 / 2)

    def test_derivatives(self):
        x = 1
        y = 2
        amp = 1. * 2 * np.pi
        center_x = 1.
        center_y = 1.
        sigma_x = 1.
        sigma_y = 1.
        values = self.Gaussian.derivatives(x, y, amp, center_x, center_y,
                                           sigma_x, sigma_y)
        assert values[0] == 0.
        assert values[1] == -np.exp(-1. / 2)
        x = np.array([2, 3, 4])
        y = np.array([1, 1, 1])
        values = self.Gaussian.derivatives(x, y, amp, center_x, center_y,
                                           sigma_x, sigma_y)
        assert values[0][0] == -np.exp(-1. / 2)
        assert values[1][0] == 0.
        assert values[0][1] == -2 * np.exp(-2.**2 / 2)
        assert values[1][1] == 0.

    def test_hessian(self):
        x = 1
        y = 2
        amp = 1. * 2 * np.pi
        center_x = 1.
        center_y = 1.
        sigma_x = 1.
        sigma_y = 1.
        values = self.Gaussian.hessian(x, y, amp, center_x, center_y, sigma_x,
                                       sigma_y)
        assert values[0] == -np.exp(-1. / 2)
        assert values[1] == 0.
        assert values[2] == 0.
        x = np.array([2, 3, 4])
        y = np.array([1, 1, 1])
        values = self.Gaussian.hessian(x, y, amp, center_x, center_y, sigma_x,
                                       sigma_y)
        assert values[0][0] == 0.
        assert values[1][0] == -np.exp(-1. / 2)
        assert values[2][0] == 0.
        assert values[0][1] == 0.40600584970983811
        assert values[1][1] == -0.1353352832366127
        assert values[2][1] == 0.
コード例 #9
0
 def setup(self):
     self.Gaussian = Gaussian()
コード例 #10
0
    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)
コード例 #11
0
    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))
コード例 #12
0
 def __init__(self):
     self.gaussian = Gaussian()
     self.ds = 0.00001
     super(LensProfileBase, self).__init__()
コード例 #13
0
class GaussianKappa(LensProfileBase):
    """
    this class contains functions to evaluate a Gaussian function and calculates its derivative and hessian matrix
    """
    param_names = ['amp', 'sigma', 'center_x', 'center_y']
    lower_limit_default = {'amp': 0, 'sigma': 0, 'center_x': -100, 'center_y': -100}
    upper_limit_default = {'amp': 100, 'sigma': 100, 'center_x': 100, 'center_y': 100}

    def __init__(self):
        self.gaussian = Gaussian()
        self.ds = 0.00001
        super(LensProfileBase, self).__init__()

    def function(self, x, y, amp, sigma, center_x=0, center_y=0):
        """
        returns Gaussian
        """
        x_ = x - center_x
        y_ = y - center_y
        r = np.sqrt(x_**2 + y_**2)
        sigma_x, sigma_y = sigma, sigma
        c = 1. / (2 * sigma_x * sigma_y)
        if isinstance(x_, int) or isinstance(x_, float):
            num_int = self._num_integral(r, c)
        else:
            num_int = []
            for i in range(len(x_)):
                num_int.append(self._num_integral(r[i], c))
            num_int = np.array(num_int)
        amp_density = self._amp2d_to_3d(amp, sigma_x, sigma_y)
        amp2d = amp_density / (np.sqrt(np.pi) * np.sqrt(sigma_x * sigma_y * 2))
        amp2d *= 2 * 1. / (2 * c)
        return num_int * amp2d

    def _num_integral(self, r, c):
        """
        numerical integral (1-e^{-c*x^2})/x dx [0..r]
        :param r: radius
        :param c: 1/2sigma^2
        :return:
        """
        out = integrate.quad(lambda x: (1-np.exp(-c*x**2))/x, 0, r)
        return out[0]

    def derivatives(self, x, y, amp, sigma, center_x=0, center_y=0):
        """
        returns df/dx and df/dy of the function
        """
        x_ = x - center_x
        y_ = y - center_y
        R = np.sqrt(x_**2 + y_**2)
        sigma_x, sigma_y = sigma, sigma
        if isinstance(R, int) or isinstance(R, float):
            R = max(R, self.ds)
        else:
            R[R <= self.ds] = self.ds
        alpha = self.alpha_abs(R, amp, sigma)
        return alpha / R * x_, alpha / R * y_

    def hessian(self, x, y, amp, sigma, center_x=0, center_y=0):
        """
        returns Hessian matrix of function d^2f/dx^2, d^f/dy^2, d^2/dxdy
        """
        x_ = x - center_x
        y_ = y - center_y
        r = np.sqrt(x_**2 + y_**2)
        sigma_x, sigma_y = sigma, sigma
        if isinstance(r, int) or isinstance(r, float):
            r = max(r, self.ds)
        else:
            r[r <= self.ds] = self.ds
        d_alpha_dr = -self.d_alpha_dr(r, amp, sigma_x, sigma_y)
        alpha = self.alpha_abs(r, amp, sigma)

        f_xx = -(d_alpha_dr/r + alpha/r**2) * x_**2/r + alpha/r
        f_yy = -(d_alpha_dr/r + alpha/r**2) * y_**2/r + alpha/r
        f_xy = -(d_alpha_dr/r + alpha/r**2) * x_*y_/r
        return f_xx, f_yy, f_xy

    def density(self, r, amp, sigma):
        """

        :param r:
        :param amp:
        :param sigma:
        :return:
        """
        sigma_x, sigma_y = sigma, sigma
        return self.gaussian.function(r, 0, amp, sigma_x, sigma_y)

    def density_2d(self, x, y, amp, sigma, center_x=0, center_y=0):
        """

        :param R:
        :param am:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        sigma_x, sigma_y = sigma, sigma
        amp2d = self._amp3d_to_2d(amp, sigma_x, sigma_y)
        return self.gaussian.function(x, y, amp2d, sigma_x, sigma_y, center_x, center_y)

    def mass_2d(self, R, amp, sigma):
        """

        :param R:
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        sigma_x, sigma_y = sigma, sigma
        amp2d = amp / (np.sqrt(np.pi) * np.sqrt(sigma_x * sigma_y * 2))
        c = 1./(2 * sigma_x * sigma_y)
        return amp2d * 2 * np.pi * 1./(2*c) * (1. - np.exp(-c * R**2))

    def mass_2d_lens(self, R, amp, sigma):
        """

        :param R:
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        sigma_x, sigma_y = sigma, sigma
        amp_density = self._amp2d_to_3d(amp, sigma_x, sigma_y)
        return self.mass_2d(R, amp_density, sigma)

    def alpha_abs(self, R, amp, sigma):
        """
        absolute value of the deflection
        :param R:
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        sigma_x, sigma_y = sigma, sigma
        amp_density = self._amp2d_to_3d(amp, sigma_x, sigma_y)
        alpha = self.mass_2d(R, amp_density, sigma) / np.pi / R
        return alpha

    def d_alpha_dr(self, R, amp, sigma_x, sigma_y):
        """

        :param R:
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        c = 1. / (2 * sigma_x * sigma_y)
        A = self._amp2d_to_3d(amp, sigma_x, sigma_y) * np.sqrt(2/np.pi*sigma_x*sigma_y)
        return 1./R**2 * (-1 + (1 + 2*c*R**2) * np.exp(-c*R**2)) * A

    def mass_3d(self, R, amp, sigma):
        """

        :param R:
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        sigma_x, sigma_y = sigma, sigma
        A = amp / (2 * np.pi * sigma_x * sigma_y)
        c = 1. / (2 * sigma_x * sigma_y)
        result = 1. /(2*c) * (-R * np.exp(-c*R**2) + scipy.special.erf(np.sqrt(c) * R) * np.sqrt(np.pi/(4 * c)))
        return result*A * 4 * np.pi

    def mass_3d_lens(self, R, amp, sigma):
        """

        :param R:
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        sigma_x, sigma_y = sigma, sigma
        amp_density = self._amp2d_to_3d(amp, sigma_x, sigma_y)
        return self.mass_3d(R, amp_density, sigma)

    def _amp3d_to_2d(self, amp, sigma_x, sigma_y):
        """
        converts 3d density into 2d density parameter
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        return amp * np.sqrt(np.pi) * np.sqrt(sigma_x * sigma_y * 2)

    def _amp2d_to_3d(self, amp, sigma_x, sigma_y):
        """
        converts 3d density into 2d density parameter
        :param amp:
        :param sigma_x:
        :param sigma_y:
        :return:
        """
        return amp / (np.sqrt(np.pi) * np.sqrt(sigma_x * sigma_y * 2))
コード例 #14
0
 def __init__(self):
     self.gaussian = Gaussian()
     self.ds = 0.00001