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20242026
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astro-ph.GA2026

pop-cosmos: Disentangling galaxy properties from observables using data-driven approaches

Benedict Van den Bussche, Sinan Deger, Hiranya V. Peiris +6

The physical processes that shape a galaxy's spectrum are strongly degenerate in observations, obscuring which processes act independently. Leveraging the pop-cosmos generative gal…

astro-ph.GA2026

pop-cosmos: Galaxy size evolution across structural and star-formation classifications in COSMOS-Web

Madalina N. Tudorache, Hiranya V. Peiris, Stephen Thorp +7

Galaxy sizes are correlated with stellar mass and redshift, as characterised by size scaling relations. The inferred forms of these scaling relations are sensitive to how galaxies…

astro-ph.GA2026

pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue

Sinan Deger, Hiranya V. Peiris, Stephen Thorp +5

We study star formation over 12 Gyr using pop-cosmos, a generative model trained on 26-band photometry of 420,000 COSMOS2020 galaxies (IRAC Ch.1 ). The model learns distributi…

astro-ph.GA2026

Spatially resolved star-formation histories of local post-starburst galaxies: Starburst and quenching spatial patterns consistent with recent mergers

Ho-Hin Leung, Vivienne Wild, Michail Papathomas +6

Post-starburst (PSB) galaxies, having recently experienced a starburst followed by rapid quenching, are excellent laboratories to probe physical mechanisms that drive starbursts an…

astro-ph.GA2026

pop-cosmos: Redshifts and physical properties of KiDS-1000 galaxies

Anik Halder, Hiranya V. Peiris, Stephen Thorp +8

Principled Bayesian inference of galaxy properties has not previously been performed for wide-area weak lensing surveys with millions of sources. We address this gap by applying th…

astro-ph.GA2025

pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population

Stephen Thorp, Hiranya V. Peiris, Gurjeet Jagwani +6

We present an extension of the pop-cosmos model for the evolving galaxy population up to redshift . The model is trained on distributions of observed colors and magnitudes,…