Fadely, Willman, and I realized today that our data-driven, hierarchical Bayesian discrete classification system for faint sources in current and future optical survey data is also a photometric redshift prediction system. We decided (tentatively) that we should write a paper on that. I also had conversations with Foreman-Mackey about Gaussian processes, and Ben Weaver (NYU) about SDSS-III BOSS redshift fitting.
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