(abs, pdf) Whalen et al., Physical Models for the Clustering of Obscured and Unobscured Quasars
(abs, pdf) Adams et al., The rest-frame UV luminosity function at $z \simeq 4$: a significant contribution of AGN to the bright-end of the galaxy population
(abs, pdf) Hughes et al., The [{\alpha}/Fe]-[Fe/H] relation in the E-MOSAICS simulations: its connection to the birth place of globular clusters and the fraction of globular cluster field stars in the bulge
(abs, pdf) Seguel et al., Formation of SMBH seeds in Pop III star clusters through collisions : the importance of mass loss
(abs, pdf) Cole & Silk, Small-scale primordial fluctuations in the 21cm Dark Ages signal
(abs, pdf) Fan et al., Alma Reveals A Gas-rich, Maximum-starburst In The Hyperluminous, Dust-obscured Quasar W0533-3401 AT $z\sim2.9$
(abs, pdf) Forrest et al., An Extremely Massive Quiescent Galaxy at $z=3.493$: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models
(abs, pdf) Jang et al., Multiple populations in globular clusters: Unified efforts from stellar evolution and chemical evolution models
(abs, pdf) Mebane et al., The Effects of Population III X-ray and Radio Backgrounds on the Cosmological 21-cm Signal
(abs, pdf) Martizzi et al., Baryons in the CosmicWeb of IllustrisTNG — II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
(abs, pdf) Hani et al., The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations
(abs, pdf) Hutter et al., The 21cm bispectrum during reionization: a tracer of the ionization topology
(abs, pdf) Besla et al., Astro2020: Training the Future Generation of Computational Researchers
(abs, pdf) Lozanov, Lectures on Reheating after Inflation
(abs, pdf) Colombo et al., Non-LTE radiation hydrodynamics in PLUTO
(abs, pdf) Gronke & Oh, How cold gas continuously entrains mass and momentum from a hot wind