Source code for lenstronomy.LightModel.Profiles.nie

import numpy as np
import lenstronomy.Util.param_util as param_util
from lenstronomy.LightModel.Profiles.profile_base import LightProfileBase

__all__ = ["NIE"]




class NIE(LightProfileBase):
    """Non-divergent isothermal ellipse (projected) This is effectively the convergence
    profile of the NIE lens model with an amplitude 'amp' rather than an Einstein radius
    'theta_E'."""

    param_names = ["amp", "e1", "e2", "s_scale", "center_x", "center_y"]
    lower_limit_default = {
        "amp": 0,
        "e1": -0.5,
        "e2": -0.5,
        "s_scale": 0,
        "center_x": -100,
        "center_y": -100,
    }
    upper_limit_default = {
        "amp": 100,
        "e1": 0.5,
        "e2": 0.5,
        "s_scale": 100,
        "center_x": 100,
        "center_y": 100,
    }



    def function(self, x, y, amp, e1, e2, s_scale, center_x=0, center_y=0):
        """

        :param x: x-coordinate
        :param y: y-coordinate
        :param amp: surface brightness normalization
        :param e1: eccentricity component
        :param e2: eccentricity component
        :param s_scale: smoothing scale (square averaged of minor and major axis)
        :param center_x: center of profile
        :param center_y: center of profile
        :return: surface brightness of NIE profile
        """
        # phi_G, q = param_util.ellipticity2phi_q(e1, e2)
        # s = s_scale * np.sqrt((1 + q ** 2) / (2 * q ** 2))
        x__, y__ = param_util.transform_e1e2_product_average(
            x, y, e1, e2, center_x, center_y
        )
        f_ = amp / 2.0 * (s_scale**2 + x__**2 + y__**2) ** (-1.0 / 2)
        return f_




    def light_3d(self, r, amp, e1, e2, s_scale, center_x=0, center_y=0):
        """3d light distribution (in spherical regime)

        :param r: 3d radius
        :param amp: surface brightness normalization
        :param e1: eccentricity component
        :param e2: eccentricity component
        :param s_scale: smoothing scale (square averaged of minor and major axis)
        :param center_x: center of profile
        :param center_y: center of profile
        :return: light density at 3d radius
        """
        rho = self._amp2rho(amp)
        return rho / (r**2 + s_scale**2)


    @staticmethod
    def _amp2rho(amp):
        """Converts surface brightness normalization 'amp' into 3d density normalization
        rho.

        :param amp:
        :return: rho
        """
        factor = np.pi
        return amp / 2 / factor