Source code for lenstronomy.LensModel.Profiles.nfw_ellipse

__author__ = "sibirrer"

import numpy as np
from lenstronomy.LensModel.Profiles.nfw import NFW
import lenstronomy.Util.param_util as param_util
from lenstronomy.LensModel.Profiles.base_profile import LensProfileBase

__all__ = ["NFW_ELLIPSE"]


[docs] class NFW_ELLIPSE(LensProfileBase): """This class contains functions concerning the NFW profile with an ellipticity defined in the potential parameterization of alpha_Rs and Rs is the same as for the spherical NFW profile. from Glose & Kneib: https://cds.cern.ch/record/529584/files/0112138.pdf relation are: R_200 = c * Rs """ profile_name = "NFW_ELLIPSE" param_names = ["Rs", "alpha_Rs", "e1", "e2", "center_x", "center_y"] lower_limit_default = { "Rs": 0, "alpha_Rs": 0, "e1": -0.5, "e2": -0.5, "center_x": -100, "center_y": -100, } upper_limit_default = { "Rs": 100, "alpha_Rs": 10, "e1": 0.5, "e2": 0.5, "center_x": 100, "center_y": 100, }
[docs] def __init__(self, interpol=False, num_interp_X=1000, max_interp_X=10): """ :param interpol: bool, if True, interpolates the functions F(), g() and h() :param num_interp_X: int (only considered if interpol=True), number of interpolation elements in units of r/r_s :param max_interp_X: float (only considered if interpol=True), maximum r/r_s value to be interpolated (returning zeros outside) """ self.nfw = NFW( interpol=interpol, num_interp_X=num_interp_X, max_interp_X=max_interp_X ) self._diff = 0.0000000001 super(NFW_ELLIPSE, self).__init__()
[docs] def function(self, x, y, Rs, alpha_Rs, e1, e2, center_x=0, center_y=0): """Returns elliptically distorted NFW lensing potential. :param x: angular position (normally in units of arc seconds) :param y: angular position (normally in units of arc seconds) :param Rs: turn over point in the slope of the NFW profile in angular unit :param alpha_Rs: deflection (angular units) at projected Rs :param e1: eccentricity component in x-direction :param e2: eccentricity component in y-direction :param center_x: center of halo (in angular units) :param center_y: center of halo (in angular units) :return: lensing potential """ x_, y_ = param_util.transform_e1e2_square_average( x, y, e1, e2, center_x, center_y ) R_ = np.sqrt(x_**2 + y_**2) rho0_input = self.nfw.alpha2rho0(alpha_Rs=alpha_Rs, Rs=Rs) if Rs < 0.0000001: Rs = 0.0000001 f_ = self.nfw.nfw_potential(R_, Rs, rho0_input) return f_
[docs] def derivatives(self, x, y, Rs, alpha_Rs, e1, e2, center_x=0, center_y=0): """Returns df/dx and df/dy of the function, calculated as an elliptically distorted deflection angle of the spherical NFW profile. :param x: angular position (normally in units of arc seconds) :param y: angular position (normally in units of arc seconds) :param Rs: turn over point in the slope of the NFW profile in angular unit :param alpha_Rs: deflection (angular units) at projected Rs :param e1: eccentricity component in x-direction :param e2: eccentricity component in y-direction :param center_x: center of halo (in angular units) :param center_y: center of halo (in angular units) :return: deflection in x-direction, deflection in y-direction """ x_, y_ = param_util.transform_e1e2_square_average( x, y, e1, e2, center_x, center_y ) phi_G, q = param_util.ellipticity2phi_q(e1, e2) cos_phi = np.cos(phi_G) sin_phi = np.sin(phi_G) e = param_util.q2e(q) # e = abs(1 - q) R_ = np.sqrt(x_**2 + y_**2) rho0_input = self.nfw.alpha2rho0(alpha_Rs=alpha_Rs, Rs=Rs) if Rs < 0.0000001: Rs = 0.0000001 f_x_prim, f_y_prim = self.nfw.nfw_alpha(R_, Rs, rho0_input, x_, y_) f_x_prim *= np.sqrt(1 - e) f_y_prim *= np.sqrt(1 + e) f_x = cos_phi * f_x_prim - sin_phi * f_y_prim f_y = sin_phi * f_x_prim + cos_phi * f_y_prim return f_x, f_y
[docs] def hessian(self, x, y, Rs, alpha_Rs, e1, e2, center_x=0, center_y=0): """Returns Hessian matrix of function d^2f/dx^2, d^f/dy^2, d^2/dxdy the calculation is performed as a numerical differential from the deflection field. Analytical relations are possible. :param x: angular position (normally in units of arc seconds) :param y: angular position (normally in units of arc seconds) :param Rs: turn over point in the slope of the NFW profile in angular unit :param alpha_Rs: deflection (angular units) at projected Rs :param e1: eccentricity component in x-direction :param e2: eccentricity component in y-direction :param center_x: center of halo (in angular units) :param center_y: center of halo (in angular units) :return: d^2f/dx^2, d^2/dxdy, d^2/dydx, d^f/dy^2 """ alpha_ra, alpha_dec = self.derivatives( x, y, Rs, alpha_Rs, e1, e2, center_x, center_y ) diff = self._diff alpha_ra_dx, alpha_dec_dx = self.derivatives( x + diff, y, Rs, alpha_Rs, e1, e2, center_x, center_y ) alpha_ra_dy, alpha_dec_dy = self.derivatives( x, y + diff, Rs, alpha_Rs, e1, e2, center_x, center_y ) f_xx = (alpha_ra_dx - alpha_ra) / diff f_xy = (alpha_ra_dy - alpha_ra) / diff f_yx = (alpha_dec_dx - alpha_dec) / diff f_yy = (alpha_dec_dy - alpha_dec) / diff return f_xx, f_xy, f_yx, f_yy
[docs] def mass_3d_lens(self, r, Rs, alpha_Rs, e1=1, e2=0): """ :param r: radius (in angular units) :param Rs: :param alpha_Rs: :param e1: :param e2: :return: """ return self.nfw.mass_3d_lens(r, Rs, alpha_Rs)
[docs] def density_lens(self, r, Rs, alpha_Rs, e1=1, e2=0): """Computes the density at 3d radius r given lens model parameterization. The integral in the LOS projection of this quantity results in the convergence quantity. :param r: 3d radios :param Rs: turn-over radius of NFW profile :param alpha_Rs: deflection at Rs :return: density rho(r) """ return self.nfw.density_lens(r, Rs, alpha_Rs)