Choose timezone
Your profile timezone:
I will describe a new self-calibration approach based on hierarchical modeling that delivers precise redshifts as well as recalibrated photometry and SED models for galaxy surveys. I will show a demonstration of this approach on early DES data, and how it opens new perspectives for the exploitation of ongoing and upcoming surveys such as LSST. I will also discuss the use of machine learning in physics, and two exciting new avenues of research: encoding physics in machine learning algorithms, and embedding machine learning in hierarchical causal models.