Light Profiles#
Standard [ag.lp]#
Standard parametric light profiles whose intensity is a free parameter of the model.
The elliptical Gaussian light profile. |
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The spherical Gaussian light profile. |
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The elliptical Gaussian light profile with m=3 and m=4 Fourier multipole perturbations on the eccentric radius. |
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The elliptical Sersic light profile. |
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The spherical Sersic light profile. |
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The elliptical Sersic light profile with m=3 and m=4 Fourier multipole perturbations on the eccentric radius. |
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The elliptical exponential profile. |
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The spherical exponential profile. |
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The elliptical Dev Vaucouleurs light profile. |
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The spherical Dev Vaucouleurs light profile. |
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The elliptical cored-Sersic light profile. |
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The elliptical cored-Sersic light profile. |
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The elliptical cored-Exponential light profile. |
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The elliptical cored-Exponential light profile. |
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The elliptical Chameleon light profile. |
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The spherical Chameleon light profile. |
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The elliptical Elson, Fall and Freeman (EFF) light profile, which is commonly used to represent the clumps of Lyman-alpha emitter galaxies (see https://arxiv.org/abs/1708.08854). |
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The spherical Elson, Fall and Freeman (EFF) light profile, which is commonly used to represent the clumps of Lyman-alpha emitter galaxies (see https://arxiv.org/abs/1708.08854). |
Linear [ag.lp_linear]#
Linear light profiles whose intensity is not a free parameter but is instead solved
analytically via a linear matrix inversion during each likelihood evaluation. This allows
many profiles to be combined efficiently without exploding the non-linear parameter space.
The elliptical Gaussian light profile. |
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The spherical Gaussian light profile. |
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The linear elliptical Gaussian light profile with m=3 and m=4 Fourier multipole perturbations on the eccentric radius. |
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The elliptical Sersic light profile. |
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The spherical Sersic light profile. |
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The linear elliptical Sersic light profile with m=3 and m=4 Fourier multipole perturbations on the eccentric radius. |
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The elliptical Exponential light profile. |
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The spherical Exponential light profile. |
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The elliptical DevVaucouleurs light profile. |
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The spherical DevVaucouleurs light profile. |
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The elliptical cored-Sersic light profile. |
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The spherical cored-Sersic light profile. |
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The elliptical cored-Exponential light profile. |
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The spherical cored-Exponential light profile. |
Operated [ag.lp_operated]#
Operated light profiles that represent emission which has already had an instrument
operation (e.g. PSF convolution) applied to it. The operated_only parameter on
fitting classes controls whether these profiles are included or excluded from a given
image computation.
Basis [ag.lp_basis]#
A Basis groups a collection of light profiles (e.g. a Multi-Gaussian Expansion or
shapelet decomposition) so that they behave as a single profile in the model. When the
constituent profiles are LightProfileLinear instances their intensities are all solved
simultaneously via a single inversion.
A basis is a collection of multiple light or mass profiles that are used to represent the light or mass distribution of a galaxy. |