(abs, pdf) Pawlowski et al., Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?
(abs, pdf) Garrison-Kimmel et al., Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment
(abs, pdf) Domínguez-Fernández et al., Dynamical evolution of magnetic fields in the intracluster medium
(abs, pdf) Carleo et al., Machine learning and the physical sciences
(abs, pdf) De Barros et al., The GREATS H$\beta$+[OIII] Luminosity Function and Galaxy Properties at $\mathbf{z\sim8}$: Walking the Way of JWST
(abs, pdf) Aung et al., Kelvin-Helmholtz Instability in Self-Gravitating Streams
(abs, pdf) Lopez et al., Supernova Remnants in High Definition
(abs, pdf) Ruszkowski et al., Supermassive Black Hole Feedback
(abs, pdf) Hodges-Kluck et al., Astro2020: Hot Drivers of Stellar Feedback from 10 to 10,000 pc
(abs, pdf) Ludlow et al., Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
(abs, pdf) Ivkovich & McCall, Denuded Dwarfs Demystified: Gas Loss from dSph Progenitors and Implications for the Minimum Mass of Galaxies
(abs, pdf) Lovell et al., Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
(abs, pdf) Yung et al., Semi-analytic forecasts for JWST – II. physical properties and scaling relations for galaxies at z = 4-10
(abs, pdf) Jung et al., Texas Spectroscopic Search for Ly$\alpha$ Emission at the End of Reionization II. The Deepest Near-Infrared Spectroscopic Observation at $z\gtrsim7$
(abs, pdf) Acquaviva, Pushing the Technical Frontier: From Overwhelmingly Large Data Sets to Machine Learning
(abs, pdf) Cooper et al., Heavy Element Absorption Systems at $5.0<z<6.8$: Metal-Poor Neutral Gas and a Diminishing Signature of Highly Ionized Circumgalactic Matter
(abs, pdf) Kimm et al., Understanding the escape of LyC and Ly$\alpha$ photons from turbulent clouds