Esempio n. 1
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    def test__1x1_image__light_profile_fits_data_perfectly__lh_is_noise(self):
        image = al.ScaledSquarePixelArray(array=np.ones((3, 3)),
                                          pixel_scale=1.0)

        noise_map = al.ScaledSquarePixelArray(array=np.ones((3, 3)),
                                              pixel_scale=1.0)

        galaxy_data = al.GalaxyData(image=image,
                                    noise_map=noise_map,
                                    pixel_scale=3.0)

        mask = al.Mask(
            array=np.array([[True, True, True], [True, False, True],
                            [True, True, True]]),
            pixel_scale=1.0,
            sub_size=1,
        )
        g0 = MockGalaxy(value=1.0)

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_image=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.model_galaxies == [g0]
        assert fit.likelihood == -0.5 * np.log(2 * np.pi * 1.0)

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_convergence=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.model_galaxies == [g0]
        assert fit.likelihood == -0.5 * np.log(2 * np.pi * 1.0)

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_potential=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.model_galaxies == [g0]
        assert fit.likelihood == -0.5 * np.log(2 * np.pi * 1.0)

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_deflections_y=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.model_galaxies == [g0]
        assert fit.likelihood == -0.5 * np.log(2 * np.pi * 1.0)

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_deflections_x=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.model_galaxies == [g0]
        assert fit.likelihood == -0.5 * np.log(2 * np.pi * 1.0)
Esempio n. 2
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    def test__deflections_y(self, gal_data_7x7, sub_mask_7x7):

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=gal_data_7x7,
                                           mask=sub_mask_7x7,
                                           use_deflections_y=True)

        galaxy = al.Galaxy(
            redshift=0.5,
            mass=al.mass_profiles.SphericalIsothermal(centre=(1.0, 2.0),
                                                      einstein_radius=1.0),
        )

        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data,
                           model_galaxies=[galaxy])

        assert fit.model_galaxies == [galaxy]

        model_data_2d = galaxy.deflections_from_grid(
            grid=galaxy_fit_data.grid,
            return_in_2d=True,
            return_binned=True,
            bypass_decorator=False,
        )[:, :, 0]

        residual_map_2d = af.fit_util.residual_map_from_data_mask_and_model_data(
            data=galaxy_fit_data.image(return_in_2d=True),
            mask=galaxy_fit_data.mask,
            model_data=model_data_2d,
        )

        assert residual_map_2d == pytest.approx(
            fit.residual_map(return_in_2d=True), 1e-4)

        chi_squared_map_2d = af.fit_util.chi_squared_map_from_residual_map_noise_map_and_mask(
            residual_map=residual_map_2d,
            mask=galaxy_fit_data.mask,
            noise_map=galaxy_fit_data.noise_map(return_in_2d=True),
        )

        assert chi_squared_map_2d == pytest.approx(
            fit.chi_squared_map(return_in_2d=True), 1e-4)

        chi_squared = af.fit_util.chi_squared_from_chi_squared_map_and_mask(
            chi_squared_map=chi_squared_map_2d, mask=sub_mask_7x7)

        noise_normalization = af.fit_util.noise_normalization_from_noise_map_and_mask(
            mask=galaxy_fit_data.mask,
            noise_map=galaxy_fit_data.noise_map(return_in_2d=True),
        )

        likelihood = af.fit_util.likelihood_from_chi_squared_and_noise_normalization(
            chi_squared=chi_squared, noise_normalization=noise_normalization)

        assert likelihood == pytest.approx(fit.likelihood, 1e-4)
Esempio n. 3
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    def test__1x2_image__noise_not_1__alls_correct(self):
        image = al.ScaledSquarePixelArray(array=5.0 * np.ones((3, 4)),
                                          pixel_scale=1.0)
        image[1, 2] = 4.0

        noise_map = al.ScaledSquarePixelArray(array=2.0 * np.ones((3, 4)),
                                              pixel_scale=1.0)

        galaxy_data = al.GalaxyData(image=image,
                                    noise_map=noise_map,
                                    pixel_scale=3.0)

        mask = al.Mask(
            array=np.array([
                [True, True, True, True],
                [True, False, False, True],
                [True, True, True, True],
            ]),
            pixel_scale=1.0,
            sub_size=1,
        )

        g0 = MockGalaxy(value=1.0, shape=2)

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_image=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])

        assert fit.model_galaxies == [g0]
        assert fit.chi_squared == (25.0 / 4.0)
        assert fit.reduced_chi_squared == (25.0 / 4.0) / 2.0
        assert fit.likelihood == -0.5 * (
            (25.0 / 4.0) + 2.0 * np.log(2 * np.pi * 2.0**2))

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_convergence=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.model_galaxies == [g0]
        assert fit.chi_squared == (25.0 / 4.0)
        assert fit.reduced_chi_squared == (25.0 / 4.0) / 2.0
        assert fit.likelihood == -0.5 * (
            (25.0 / 4.0) + 2.0 * np.log(2 * np.pi * 2.0**2))

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_potential=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.model_galaxies == [g0]
        assert fit.chi_squared == (25.0 / 4.0)
        assert fit.reduced_chi_squared == (25.0 / 4.0) / 2.0
        assert fit.likelihood == -0.5 * (
            (25.0 / 4.0) + 2.0 * np.log(2 * np.pi * 2.0**2))

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_deflections_y=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.chi_squared == (25.0 / 4.0)
        assert fit.reduced_chi_squared == (25.0 / 4.0) / 2.0
        assert fit.likelihood == -0.5 * (
            (25.0 / 4.0) + 2.0 * np.log(2 * np.pi * 2.0**2))

        galaxy_fit_data = al.GalaxyFitData(galaxy_data=galaxy_data,
                                           mask=mask,
                                           use_deflections_x=True)
        fit = al.GalaxyFit(galaxy_data=galaxy_fit_data, model_galaxies=[g0])
        assert fit.chi_squared == (25.0 / 4.0)
        assert fit.reduced_chi_squared == (25.0 / 4.0) / 2.0
        assert fit.likelihood == -0.5 * (
            (25.0 / 4.0) + 2.0 * np.log(2 * np.pi * 2.0**2))
Esempio n. 4
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def make_gal_fit_7x7_deflections_x(gal_fit_data_7x7_deflections_x, gal_x1_mp):
    return al.GalaxyFit(galaxy_data=gal_fit_data_7x7_deflections_x,
                        model_galaxies=[gal_x1_mp])
Esempio n. 5
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def make_gal_fit_7x7_potential(gal_fit_data_7x7_potential, gal_x1_mp):
    return al.GalaxyFit(galaxy_data=gal_fit_data_7x7_potential,
                        model_galaxies=[gal_x1_mp])
Esempio n. 6
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def make_gal_fit_7x7_convergence(gal_fit_data_7x7_convergence, gal_x1_mp):
    return al.GalaxyFit(galaxy_data=gal_fit_data_7x7_convergence,
                        model_galaxies=[gal_x1_mp])
Esempio n. 7
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def make_gal_fit_7x7_image(gal_fit_data_7x7_image, gal_x1_lp):
    return al.GalaxyFit(galaxy_data=gal_fit_data_7x7_image,
                        model_galaxies=[gal_x1_lp])