Tom Charnock
Institut d'Astrophysique de Paris
The generator $({\bf d}\in\mathcal{M}(\boldsymbol{\theta}))$ of data $({\bf d})$ with model parameters $(\boldsymbol{\theta})$
Impossibly large numbers of simulations become necessary to correctly sample the posterior

*in the optimal case...
$$\boldsymbol{\theta}^\textsf{MLE}_\alpha=\boldsymbol{\theta}_\alpha^*+{\bf F}_{\alpha\beta}^{-1}{\bf C}_\mathscr{f}^{-1}\frac{\partial\mu_\mathscr{f}}{\partial\theta_\beta}({\bf x}-\mu_\mathscr{f})$$
$$\textsf{Cov}[\boldsymbol{\theta}_\alpha^\textsf{MLE},\boldsymbol{\theta}_\beta^\textsf{MLE}] \ge {\bf F}_{\alpha\beta}^{-1}$$
Compare distance between observed summaries and simulation summaries and select results within $\epsilon$


Build networks using physical principles.
Reduces number of parameters
Increases computational efficiency
Decreases overfitting
Improves interpretability
$$\begin{align*}
{\Tiny\mathcal{L} =}&{\Tiny \sum_{j\in\textsf{catalogue}}\log\left[\sum_i^N\frac{\alpha_{i,j}}{\sqrt{2\pi\sigma_{i,j}^2}}\textsf{exp}\left[-\frac{\left(\textsf{ln}(M_j) - \mu_{i,j}\right)^2}{2\sigma_{i,j}^2}\right]\right]}\\
&{\Tiny - V\sum_{j\in\textsf{voxels},i=1}^N\frac{\alpha_{i,j}}{2}\textsf{exp}\left[\frac{\sigma_{i,j}^2}{2}\right]\textsf{erfc}\left[\frac{\textsf{ln}\left(M_\textsf{th}\right) - \mu_{i,j} - \sigma_{i,j}^2}{\sqrt{2\sigma_{i,j}^2}}\right].}
\end{align*}$$
Nearly impossible to know the mass matrix, ${\bf M}$.
✓ Weight values are properly sampled after burn in
✓ NPE acts as a contrast enhancer
✓ Fits data!
Stop doing machine learning, think, then start doing machine learning again!