
Cosmological Mass Maps
Astronomers seek to use mass maps collected via telescopes to infer cosmological parameters governing the initial state of the universe, such as energy density \((\Omega_m)\) and matter fluctuations \((\sigma_8)\). While deep networks can use cosmological simulations to predict well at this task, explanations thereof can potentially draw attention to new patterns and discoveries if they are understandable to cosmologists. Explanations of mass map predictions that are aligned with cosmological structures (e.g. voids and clusters) can potentially advance our understanding of the formation of the universe.




