NumPy/SciPy#
See Units, shapes and model contracts for units, shapes, domains and backend boundaries, and Quickstart for executable minimal examples.
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Subclassing interface for spherical anisotropy. |
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Baes--van Hese spherical anisotropy with numerical LOS quadrature. |
Convert a numerical J factor from Msun^2/pc^5 to GeV^2/cm^5. |
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Constant spherical anisotropy beta(r)=beta_ani. |
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Base class for NumPy/SciPy dark-matter density profiles. |
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Composite spherical Jeans model for dwarf spheroidal systems. |
Dictionary with attribute access to existing keys. |
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Stellar model with an exponential projected surface density. |
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Subclassing interface for stateful likelihoods and prior terms. |
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Finite uniform bounds in explicitly named sampling coordinates. |
Solar gravitational parameter G*Msun, in m^3/s^2. |
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Base class for stateful NumPy/SciPy model components. |
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Spherical NFW halo with a hard density cutoff at |
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Osipkov--Merritt spherical anisotropy with an analytic kernel. |
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Lightweight mapping used for stateful model parameters. |
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Gaussian prior for |
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Unit-integral Plummer tracer; re_pc is its projected half-light radius. |
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Projected Sérsic stellar model with selectable 3-D deprojection. |
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Spherical Jeans inference with a Gaussian LOS-velocity likelihood. |
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Base class for projected/deprojected stellar-density models. |
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Unit-integral uniform projected disk with radius |
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General Zhao profile. |
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Compose Plummer + NFW + constant anisotropy with explicit finite priors. |
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Compose a NumPy tracer, halo and anisotropy into an axisymmetric model. |
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Unbinned Gaussian LOS inference with the emcee sampler interface. |
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Finite matching 1-D observations, in pc and km/s, copied on construction. |
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Unit-integral spheroidal Plummer tracer (re_pc is equatorial scale). |
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rho=rhos_Msunpc3 (m/rs_pc)^(-gamma) [1+(m/rs_pc)^alpha]^((gamma-beta)/alpha). |
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Constant cylindrical anisotropy with finite beta_z < 1. |
Interface for a normalized axisymmetric stellar tracer. |
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Interface for a spheroidal dark-matter density and gravitational field. |
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Interface for meridional anisotropy, beta_z = 1 - <vz²>/<vR²>. |