Arguably the simplest lens model is a point mass (Schwarzschild) lens, which is described by two parameters, namely, mass ($M$) and source position ($y$). The $(\psi, \hat{\alpha}, \kappa)$ for a point mass lens are given as,

\[\begin{align*} \psi(\theta) &= \theta_E^2 \ln(\theta), \\ \hat{\alpha}(\theta) &= \frac{\theta_E^2}{\theta}, \\ \kappa(\theta) &= \frac{M}{\Sigma_{\rm cr}} \delta(\theta), \end{align*}\]

where $\theta_E$ is the Einstein angle, which is given as,

\[\begin{equation*} \theta_E = \sqrt{\frac{4{\rm G}M}{\rm c^2} \frac{D_{ds}}{D_d D_s}}. \end{equation*}\]

LensFactory.Lenses.PointLens.jacobian!Function
jacobian!(ψxx::T, ψyy::T, ψxy::T, θx::T, θy::T, D_d::RV, θxc::RV, θyc::RV, mass::RV) where T <: RV
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jacobian!(ψxx::T, ψyy::T, ψxy::T, θx::T, θy::T, D_d::RV, θxc::RV, θyc::RV, mass::RV) where T <: ROA
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