The SIE lens is defined by the convergence
where is the ratio between the minor and major axes.
The magnification matrix for SIE may now be calculated Kormann 1994
and becomes $$ \mathcal{A}(\boldsymbol{\theta})¶
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where $(\xi,\phi)$ are the polar coordinates of the normalised screen space point
$\mathbf{x}$.
Now the critical curve is given as the points $(\xi_{\mathrm{crit}},\phi)$ given as\xi_{\mathrm{crit}} = \frac{\sqrt{f}\xi_0}{\sqrt{\cos^2\phi+f^2\sin^2\phi}}, $$