Tag Archives: Method

19 Feb 2020

  • (abs, pdf) Ronconi et al., ScamPy — A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
  • (abs, pdf) Takeo et al., Hyper-Eddington accretion flows onto black holes accompanied by powerful outflows
  • (abs, pdf) Davé et al., Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations

31 Jan 2020

  • (abs, pdf) Inayoshi et al., Universal transition diagram from dormant to actively accreting supermassive black holes
  • (abs, pdf) Lucchesi et al., Homogeneity in the early chemical evolution of the Sextans dwarf Spheroidal galaxy
  • (abs, pdf) Cen, Physics of Prodigious Lyman Continuum Leakers
  • (abs, pdf) Stevance et al., Hoki: Making BPASS accessible through Python
  • (abs, pdf) Visbal et al., Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization
  • (abs, pdf) Li et al., ART$^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
  • (abs, pdf) Michel-Dansac et al., RASCAS: RAdiation SCattering in Astrophysical Simulations

30 Jan 2020

  • (abs, pdf) Pizzati et al., Outflows and extended [CII] halos in high redshift galaxies
  • (abs, pdf) Izquierdo-Villalba et al., From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
  • (abs, pdf) White et al., The Structure of Radiatively Inefficient Black Hole Accretion Flows
  • (abs, pdf) Kumamoto et al., Merger rate density of binary black holes formed in open clusters
  • (abs, pdf) Mignon-Risse et al., A new hybrid radiative transfer method for massive star formation

07 Jan 2020

  • (abs, pdf) Tilvi et al., Onset of Cosmic Reionization: Evidence of An Ionized Bubble Merely 680 Myrs after the Big Bang
  • (abs, pdf) Emsenhuber et al., Realistic On-the-fly Outcomes of Planetary Collisions II: Bringing Machine Learning to N-body Simulations
  • (abs, pdf) Komiya et al., Are Faint Supernovae Responsible for Carbon-Enhanced Metal-Poor Stars?
  • (abs, pdf) Negrello et al., Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey