Tag Archives: Method

18 May 2022

  • (abs, pdf) Chiaki & Wise, Triggered Population III star formation: the effect of H$_2$ self-shielding
  • (abs, pdf) Schatz et al., Horizons: Nuclear Astrophysics in the 2020s and Beyond
  • (abs, pdf) Piras et al., Fast and realistic large-scale structure from machine-learning-augmented random field simulations
  • (abs, pdf) Ricotti et al., Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
  • (abs, pdf) Zier & Springel, Simulating cold shear flows on a moving mesh
  • (abs, pdf) Seitova & Pober, The Optical Depth of Foregrounds for the Highest Redshift 21 cm Signals

21 Apr 2022

  • (abs, pdf) Naidu et al., Live Fast, Die $\alpha$-Enhanced: The Mass-Metallicity-$\alpha$ Relation of the Milky Way's Disrupted Dwarf Galaxies
  • (abs, pdf) Collins et al., Pegasus V — a newly discovered ultra-faint dwarf galaxy on the outskirts of Andromeda
  • (abs, pdf) Klepitko et al., Tree-based solvers for adaptive mesh refinement code FLASH — III: a novel scheme for radiation pressure on dust and gas and radiative transfer from diffuse sources

13 Apr 2022

  • (abs, pdf) Weinberger & Hernquist, Modeling multi-phase gases in cosmological simulations using compressible multi-fluid hydrodynamics
  • (abs, pdf) Rizzo et al., Dynamical characterization of galaxies up to $z \sim 7$
  • (abs, pdf) Gnedin, Cosmic Reionization on Computers: Physical Origin of Long Dark Gaps in Quasar Absorption Spectra
  • (abs, pdf) Forbes et al., Gas Accretion Can Drive Turbulence in Galaxies
  • (abs, pdf) Kušmić et al., Assuming Ionization Equilibrium and the Impact on the Lyman-$\mathrm{\alpha}$ Forest Power Spectrum during the End of Reionization at $8 \geq z \geq 5$

22 Mar 2022

  • (abs, pdf) Li et al., On the Connection between Supermassive Black Hole and Galaxy Growth in the Reionization Epoch
  • (abs, pdf) Kaur et al., The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray binaries
  • (abs, pdf) Rodriguez-Gomez et al., Galactic angular momentum in the IllustrisTNG simulation — I. Connection to morphology, halo spin, and black hole mass
  • (abs, pdf) Munive-Villa et al., Solving the Schrodinger Poisson System using the coordinate Adaptive Moving Mesh method