A new statistical formalism and GPU prototype PELARGIR enable joint inference of resolved LISA sources, the Galactic binary foreground, and their shared astrophysical population inside the global fit.
instance, a population-level model allows us to compare the relative probability of a massive BH+BH in the far reaches of the Galactic disk (lower) vs
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A Foundation for Gravitational-Wave Population Inference within the LISA Global Fit
A new statistical formalism and GPU prototype PELARGIR enable joint inference of resolved LISA sources, the Galactic binary foreground, and their shared astrophysical population inside the global fit.