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https://stockholmuniversity.zoom.us/j/530682073
The next generation of galaxy surveys is aiming at combinations of
multiple tracers and even different messengers as a tool to map cosmic structures. I will discuss the advantages and limitations of the multi-tracer
technique, and some new results in the context of the natural
framework for observations -- the past light cone.
I will also present some interesting new results and perspectives for
machine learning in the realm of astrophysics and cosmology.