A score-based diffusion generative model on deep infrared galaxy photometry yields a star formation rate density peaking at z=1.3 and shows distinct non-parametric star formation histories plus AGN activity peaking during the quenching transition of massive galaxies.
@doi [ ] 10.48550/arXiv.2203.02041, https://ui.adsabs.harvard.edu/abs/1980FCPh....5..287T 5
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