(abs, pdf) Wu et al., On the accuracy of common moment-based radiative transfer methods for simulating reionization
(abs, pdf) Sanders et al., The MOSDEF Survey: The Evolution of the Mass-Metallicity Relation from $z=0$ to $z\sim3.3$
(abs, pdf) Whitney et al., Surface Brightness Evolution of Galaxies in the CANDELS GOODS Fields up to $z \sim 6$: High-z Galaxies are Unique or Remain Undetected
(abs, pdf) Ananna et al., Accretion History of AGN III: Radiative Efficiency and AGN Contribution to Reionization
(abs, pdf) Peroux et al., Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
(abs, pdf) Leslie et al., The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim5$
(abs, pdf) Esmerian et al., Thermal Instability in the CGM of $L_{\star}$ Galaxies: Testing "Precipitation" Models with the FIRE Simulations
(abs, pdf) Stern et al., Virialization of the inner CGM in the FIRE simulations and implications for galaxy discs, star formation and feedback
(abs, pdf) Ploeckinger & Schaye, Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
(abs, pdf) McKee et al., Magnetic Fields in the Formation of the First Stars. I. Theory vs. Simulation
(abs, pdf) Davies et al., Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
(abs, pdf) Yang et al., P\={o}niu\={a}'ena: A Luminous $z=7.5$ Quasar Hosting a 1.5 Billion Solar Mass Black Hole
(abs, pdf) Meng & Gnedin, Evolution of Disc Thickness in High-Redshift Galaxies
(abs, pdf) Habouzit et al., Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
(abs, pdf) Ma et al., The contribution of globular clusters to cosmic reionization
(abs, pdf) Bennett & Sijacki, Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
(abs, pdf) Sorini et al., Simba: The average properties of the circumgalactic medium of $2 \leq z \leq 3$ quasars are determined primarily by stellar feedback