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so oh this is thats already started okay hi everyone im george apollina and im a postdoctoral researcher at the university observatory oopsie in munich and you might have heard my name associated to some of these institutions or efforts but today im gonna talk about emulating the void density profile and white sides function through gaussian processes so the motivation for this kind of work is pretty straightforward voids have gained a lot of oh sorry thanks a lot of popularity as cosmological probes but were still missing some of these very simple tools to predict their zeroth and first order statistics meaning we are missing something that is just like giving a a set of cosmological parameters we just push a button that in this case is going to be an emulator based on an aggression process oh okay i have a tuple here but fine and this would give us uh directly the void size function and similarly given a cosmology and a typical void size by pushing another button we can get how
