(abs , pdf ) Borukhovetskaya et al., The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
(abs , pdf ) Chen et al., Dynamical Friction Modeling of Massive Black Holes in Cosmological Simulations and Effects on Merger Rate Predictions
(abs , pdf ) Davies & Furlanetto, Improved treatments of the ionizing photon mean free path in semi-numerical simulations of reionization
(abs , pdf ) Keller, Is There a Missing Outskirts Problem? Stellar Haloes as a Sensitive Probe of Supernova Feedback
(abs , pdf ) Rossi et al., Ultra-faint dwarf galaxies: unveiling the minimum mass of the first stars
(abs , pdf ) Reichart, Robotic Telescope Labs for Survey-Level Undergraduates
(abs , pdf ) Minniti et al., Discovery of new globular clusters in the Sagittarius dwarf galaxy
(abs , pdf ) Ghara et al., Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
(abs , pdf ) Mackey et al., PION: Simulating bow shocks and circumstellar nebulae
(abs , pdf ) Bland-Hawthorn et al., Quantum memories and the double-slit experiment: implications for astronomical interferometry
(abs , pdf ) Woosley & Heger, The Pair-Instability Mass Gap for Black Holes
(abs , pdf ) Efstathiou et al., A hyperluminous obscured quasar at a redshift of z ~ 4.3
(abs , pdf ) Kehrig et al., On the contribution of the X-ray source to the extended nebular HeII emission in IZw18
(abs , pdf ) Kretschmer et al., On the origin of surprisingly cold gas discs in galaxies at high redshift
(abs , pdf ) Pandya et al., Characterizing mass, momentum, energy and metal outflow rates of multi-phase galactic winds in the FIRE-2 cosmological simulations
(abs , pdf ) Gelles et al., The Role of Adaptive Ray Tracing in Analyzing Black Hole Structure
(abs , pdf ) Stefanon et al., Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time
(abs , pdf ) Kimbrell et al., The Diverse Morphologies and Structures of Dwarf Galaxies Hosting Optically-Selected Active Massive Black Holes
(abs , pdf ) Di Cintio et al., Pericentric passage-driven star formation in satellite galaxies and their hosts: CLUES from Local Group simulations
(abs , pdf ) Fujii et al., SIRIUS Project. III. Star-by-star simulations of star cluster formation using a direct N-body integrator with stellar feedback
(abs , pdf ) Gillet et al., 21cm signal predictions at Cosmic Dawn and Reionization with coupled radiative-hydrodynamics
(abs , pdf ) Wang et al., UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
(abs , pdf ) Collins et al., Andromeda XXI — a dwarf galaxy in a low density dark matter halo
(abs , pdf ) Ceverino et al., FirstLight IV: Diversity in sub-L$_*$ galaxies at cosmic dawn
(abs , pdf ) Bellovary et al., The Origins of Off-Center Massive Black Holes in Dwarf Galaxies
(abs , pdf ) Shen et al., Dissipative Dark Matter on FIRE: I. Structural and kinematic properties of dwarf galaxies
(abs , pdf ) Lochhaas et al., Figuring Out Gas & Galaxies In Enzo (FOGGIE) V: The Virial Temperature Does Not Describe Gas in a Virialized Galaxy Halo
(abs , pdf ) Reichert et al., Extreme r-process enhanced stars at high metallicity in Fornax
(abs , pdf ) Chan et al., Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
(abs , pdf ) Berzin et al., Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
(abs , pdf ) Chan et al., Narrowing the mass range of Fuzzy Dark Matter with Ultra-faint Dwarfs
(abs , pdf ) Dawson et al., A self-supervised, physics-aware, Bayesian neural network architecture for modelling galaxy emission-line kinematics
(abs , pdf ) Baxter et al., A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
(abs , pdf ) Lupi et al., Forming massive seed black holes in high-redshift quasar host progenitors
(abs , pdf ) Chandra & Schlaufman, Searching for Low-mass Population III Stars Disguised as White Dwarfs
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