(abs, pdf) Nori et al., Fuzzy Aquarius: evolution of a Milky-way like system in the Fuzzy Dark Matter scenario
(abs, pdf) Kim et al., Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
(abs, pdf) Yoon et al., ALMA Observation of a $z\gtrsim10$ Galaxy Candidate Discovered with JWST
(abs, pdf) Nagele et al., Pulsations of primordial supermassive stars induced by a general relativistic instability; visible to JWST at z$>$12
(abs, pdf) Balu et al., Thermal and Reionisation History within a Large-volume Semi-Analytic Galaxy Formation Simulation
(abs, pdf) Katz et al., Two Modes of LyC Escape From Bursty Star Formation: Implications for [C II] Deficits and the Sources of Reionization
(abs, pdf) Larkin et al., Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
(abs, pdf) Deng et al., Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum
(abs, pdf) Zhu et al., Gas Cooling in Hydrodynamic Simulations with An Exact Time Integration Scheme
(abs, pdf) Krumholz et al., A Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport
(abs, pdf) Amaro-Seoane et al., Sowing the seeds of massive black holes in small galaxies: Young clusters as the building blocks of Ultra-Compact-Dwarf Galaxies
(abs, pdf) Ellis et al., The Abundance of Star-Forming Galaxies in the Redshift Range 8.5 to 12: New Results from the 2012 Hubble Ultra Deep Field Campaign
(abs, pdf) Volonteri & Ciotti, Massive black holes in central cluster galaxies
(abs, pdf) Hirano & Yoshida, Radiative cooling implementations in simulations of primordial star formation
(abs, pdf) Haas et al., Physical properties of simulated galaxy populations at z=2 — II. Effects of physics ingredients other than cooling and outflows
(abs, pdf) Norris et al., The Most Metal-Poor Stars. IV. The Two Populations With [Fe/H] < -3.0