(abs , pdf ) Molaro et al., ARTIST: Fast radiative transfer for large-scale simulations of the epoch of reionisation
(abs , pdf ) Safarzadeh & Loeb, An upper limit on primordial magnetic fields from ultra-faint dwarf galaxies
(abs , pdf ) Schauer et al., Constraining First Star Formation with 21cm-Cosmology
(abs , pdf ) Grassi et al., The challenges of modelling microphysics: ambipolar diffusion, chemistry, and cosmic rays in MHD shocks
(abs , pdf ) Levy, Simulating fluids with a computer: Introduction and recent advances
(abs , pdf ) Avilez-Lopez & Guzman, Relaxation of structures resulting from head-on mergers of ultralight bosonic dark matter cores
(abs , pdf ) Donnari et al., The star-formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
(abs , pdf ) Shafieloo et al., Will Gravitational Wave Sirens Determine the Hubble Constant?
(abs , pdf ) Izotov et al., J1234+3901: an extremely metal-deficient compact star-forming dwarf galaxy at redshift 0.133
(abs , pdf ) Baumschlager et al., Refueled and shielded – The early evolution of Tidal Dwarf Galaxies
(abs , pdf ) Budiardja & Cardall, Targeting GPUs with OpenMP Directives on Summit: A Simple and Effective Fortran Experience
(abs , pdf ) Trayford & Schaye, Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
(abs , pdf ) Kodama & Ishiyama, Acceleration of the tree method with SIMD instruction set
(abs , pdf ) Emsellem et al., The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: I. Kinematics of the stellar body
(abs , pdf ) Fensch et al., The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: II. The population of DF2: stars, clusters and planetary nebulae
(abs , pdf ) Jana et al., Radio background and IGM heating due to Pop III supernovae explosions
(abs , pdf ) Leung et al., The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy
(abs , pdf ) Neeleman et al., [CII] 158 Micron Emission from z~4 HI Absorption-Selected Galaxies
(abs , pdf ) Jeon & Bromm, Signature of the first galaxies in JWST deep field observations
(abs , pdf ) Ivkovic & Teyssier, ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
(abs , pdf ) Thi et al., Warm dust surface chemistry. H2 and HD formation
(abs , pdf ) Nelson et al., The IllustrisTNG Simulations: Public Data Release
(abs , pdf ) Buck et al., A conclusive test for star formation prescriptions in cosmological hydrodynamical simulations
(abs , pdf ) Digby et al., The star formation histories of dwarf galaxies in Local Group cosmological simulations
(abs , pdf ) Allen et al., Constraining Scatter in the Stellar Mass–Halo Mass Relation for Haloes Less Massive than the Milky Way
(abs , pdf ) Ludlow et al., Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
(abs , pdf ) Benson et al., Halo concentrations from extended Press-Schechter merger histories
(abs , pdf ) Su et al., Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
(abs , pdf ) Bassett et al., On the Lack of Correlation Between [OIII]/[OII] and Lyman-Continuum Escape Fraction
(abs , pdf ) Donnert et al., WENO-Wombat: Scalable Fifth-Order Constrained-Transport Magnetohydrodynamics for Astrophysical Applications
(abs , pdf ) Pavesi et al., Low star formation efficiency in typical galaxies at z=5-6
(abs , pdf ) Marassi et al., Supernova dust yields: the role of metallicity, rotation, and fallback
(abs , pdf ) Minoda et al., Insight into Primordial Magnetic Fields from 21-cm line observation with EDGES experiment
(abs , pdf ) Goz et al., Astrophysical code migration into Exascale Era
(abs , pdf ) Diaz-Santos et al., The Multiple Merger Assembly of a Hyper-luminous Obscured Quasar at redshift 4.6
(abs , pdf ) Stoyanovskaya et al., Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation
(abs , pdf ) He et al., Learning to Predict the Cosmological Structure Formation
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