autogalaxy.profiles.light_and_mass_profiles.SersicGradientSph#
- class SersicGradientSph[source]#
Bases:
SersicGradient,LightMassProfileThe spherical Sersic light and mass profile, with a radial gradient in the conversion of light to mass..
This simultaneously represents the luminous emission and stellar mass of a galaxy.
- Parameters:
centre (
Tuple[float,float]) – The (y,x) arc-second coordinates of the profile centre.intensity (
float) – Overall flux intensity normalisation in the light profiles (electrons per second)effective_radius (
float) – The radius containing half the light of this light profile.sersic_index (
float) – The concentration of the light profilesmass_to_light_ratio (
float) – The mass-to-light ratio of the light profilesmass_to_light_gradient (
float) – The mass-to-light radial gradient.
Methods
angleThe position angle in degrees of the major-axis of the ellipse defined by profile, defined counter clockwise from the positive x-axis (0.0 > angle > 180.0).
angle_radiansThe position angle in radians of the major-axis of the ellipse defined by profile, defined counter clockwise from the positive x-axis (0.0 > angle > 2pi).
angle_to_profile_grid_fromThe angle between each angle theta on the grid and the profile, in radians.
axis_ratioThe ratio of the minor-axis to major-axis (b/a) of the ellipse defined by profile (0.0 > q > 1.0).
blurred_image_2d_fromEvaluate the light object's 2D image from a input 2D grid of coordinates and convolve it with a PSF.
convergence_2d_fromCalculate the projected convergence at a given set of arc-second gridded coordinates.
convergence_2d_via_cse_fromCalculate the projected 2D convergence from a grid of (y,x) arc second coordinates, by computing and summing the convergence of each individual cse used to decompose the mass profile.
convergence_cse_1d_fromOne dimensional function which is solved to decompose a convergence profile in cored steep ellipsoids, given by equation (14) of Oguri 2021 (https://arxiv.org/abs/2106.11464).
convergence_funcReturns the convergence of the mass profile as a function of the radial coordinate.
decompose_convergence_via_cseDecompose the convergence of the Sersic profile into singular isothermal elliptical (sie) profiles.
decompose_convergence_via_mgedeflections_2d_via_cse_fromCalculate the projected 2D deflection angles from a grid of (y,x) arc second coordinates, by computing and summing the convergence of each individual cse used to decompose the mass profile.
deflections_2d_via_potential_2d_fromReturns the 2D deflection angles of the mass profile by numerically differentiating the lensing potential on the input grid.
deflections_via_cse_fromReturns the deflection angles of a 1d cored steep ellisoid (CSE) profile, given by equation (19) and (20) of Oguri 2021 (https://arxiv.org/abs/2106.11464).
deflections_yx_2d_fromReturns the 2D deflection angles of the mass profile from a 2D grid of Cartesian (y,x) coordinates.
density_between_circular_annuliCalculate the mass between two circular annuli and compute the density by dividing by the annuli surface area.
eccentric_radii_grid_fromConvert a grid of (y,x) coordinates to an eccentric radius: :math: axis_ratio^0.5 (x^2 + (y^2/q))^0.5
elliptical_radii_grid_fromConvert a grid of (y,x) coordinates to their elliptical radii values: :math: (x^2 + (y^2/q))^0.5
extract_attributeReturns an attribute of a class and its children profiles in the galaxy as a ValueIrregular or Grid2DIrregular object.
hasReturns True if any attribute of this profile is an instance of the input class cls, else False.
image_2d_fromReturns the Sersic light profile's 2D image from a 2D grid of Cartesian (y,x) coordinates.
image_2d_via_radii_fromReturns the 2D image of the Sersic light profile from a grid of coordinates which are the radial distances of each coordinate from the its centre.
luminosity_integralRoutine to integrate the luminosity of an elliptical light profile.
luminosity_within_circle_fromIntegrate the light profile to compute the total luminosity within a circle of specified radius.
mass_angular_within_circle_fromIntegrate the mass profiles's convergence profile to compute the total mass within a circle of specified radius.
mass_integralIntegrand used by mass_angular_within_circle_from to compute the total projected mass within a circle.
padded_image_2d_fromEvaluate the light object's 2D image from a input 2D grid of padded coordinates, where this padding is sufficient to encapsulate all surrounding pixels that will blur light into the original image given the 2D shape of the PSF's kernel.
potential_2d_fromReturns the 2D lensing potential of the mass profile from a 2D grid of Cartesian (y,x) coordinates.
potential_funcReturns the integrand of the lensing potential at a single point, used in numerical integration schemes for computing the potential from the mass profile's convergence.
radial_deflection_fromradial_grid_fromConvert a grid of (y, x) coordinates, to their radial distances from the profile centre (e.g. :math: r = sqrt(x**2 + y**2)).
rotated_grid_from_reference_frame_fromRotate a grid of (y,x) coordinates which have been transformed to the elliptical reference frame of a profile back to the original unrotated coordinate grid reference frame.
transformed_from_reference_frame_grid_fromTransform a grid of (y,x) coordinates from the reference frame of the profile to the original observer reference frame.
transformed_to_reference_frame_grid_fromTransform a grid of (y,x) coordinates to the reference frame of the profile.
unmasked_blurred_image_2d_fromEvaluate the light object's 2D image from a input 2D grid of coordinates and convolve it with a PSF, using a grid which is not masked.
visibilities_fromEvaluate the light object's 2D image from a input 2D grid of coordinates and transform this to an array of visibilities using a autoarray.operators.transformer.Transformer object and therefore a Fourier Transform.
vmapped_deflections_fromAttributes
average_convergence_of_1_radiusThe radius a critical curve forms for this mass profile, e.g. where the mean convergence is equal to 1.0.
coefficient_tagA short string tag used to label the intensity coefficient when this profile is used inside a Basis object (e.g. for multi-Gaussian expansion or shapelet decomposition).
elliptical_effective_radiusThe effective_radius of a Sersic light profile is defined as the circular effective radius, which is the radius within which a circular aperture contains half the profile's total integrated light.
ellipticity_rescaleA rescaling factor applied to account for the ellipticity of the mass profile when computing the Einstein radius from the average convergence equals unity criterion.
half_light_radiusThe radius that contains half of the total light of the profile (the half-light radius).
sersic_constantA parameter derived from Sersic index which ensures that effective radius contains 50% of the profile's total integrated light.