The physical processes responsible for shaping how galaxies form and quench over time
leave imprints on both the spatial (galaxy morphology) and temporal (star formation history; …

We successfully demonstrate the use of explainable artificial intelligence (XAI) techniques
on astronomical data sets in the context of measuring galactic bar lengths. The method …

Nonparametric star formation histories (SFHs) have long promised to be the" gold standard"
for galaxy spectral energy distribution (SED) modeling as they are flexible enough to …

Galaxy morphologies provide valuable insights into their formation processes, tracing the
spatial distribution of ongoing star formation and encoding signatures of dynamical …

We introduce a novel machine-learning framework for estimating the Bayesian posteriors of
morphological parameters for arbitrarily large numbers of galaxies. The Galaxy Morphology …

Abstract We use the Galaxy Morphology Posterior Estimation Network (GaMPEN) to
estimate morphological parameters and associated uncertainties for∼ 8 million galaxies in …

We examine morphology-separated color–mass diagrams to study the quenching of star
formation in∼ 100,000 (z∼ 0) Sloan Digital Sky Survey (SDSS) and∼ 20,000 (z∼ 1) …

Galaxy morphology and its evolution over the cosmic epoch hold important clues for
understanding the regulation of star formation (SF). However, studying the relationship …

Hydrodynamical simulations of galaxy formation and evolution attempt to fully model the
physics that shapes galaxies. The agreement between the morphology of simulated and real …

Galaxy morphology is a fundamental quantity, which is essential not only for the full
spectrum of galaxy-evolution studies, but also for a plethora of science in observational …