Tag Archives: Method

10 Nov 2022

  • (abs, pdf) Riaz et al., Formation of metal-free binaries: Impact of H$_{2}$ line cooling and CIE cooling
  • (abs, pdf) Santos-Santos et al., Planes of satellites around simulated disk galaxies II: Time-persistent planes of kinematically-coherent satellites in $\Lambda$CDM
  • (abs, pdf) Chaikin et al., A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
  • (abs, pdf) Katz et al., PRISM: A Non-Equilibrium, Multiphase Interstellar Medium Model for Radiation Hydrodynamics Simulations of Galaxies
  • (abs, pdf) Kobayashi et al., Can neutron star mergers alone explain the r-process enrichment of the Milky Way?
  • (abs, pdf) Andrianomena et al., Emulating cosmological multifields with generative adversarial networks
  • (abs, pdf) Talei et al., Coupling Semi-Analytic and N-body Galaxies (CoSANG) for cosmological stellar halo simulations I- Methods and the structure of dark matter halos

07 Nov 2022

  • (abs, pdf) Trussler et al., On the observability and identification of Population III galaxies with JWST
  • (abs, pdf) Williams et al., The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
  • (abs, pdf) Lin et al., Low Metallicity Galaxies from the Dark Energy Survey
  • (abs, pdf) Popovas, DISPATCH methods: an approximate, entropy-based Riemann solver for ideal magnetohydrodynamics
  • (abs, pdf) Bagley et al., CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results
  • (abs, pdf) Liu et al., Coherent and incoherent structures in fuzzy dark matter halos
  • (abs, pdf) Bouwens et al., Evolution of the UV LF from z~15 to z~8 Using New JWST NIRCam Medium-Band Observations over the HUDF/XDF

02 Nov 2022

  • (abs, pdf) Engler et al., Satellites of MW/M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
  • (abs, pdf) Ramesh et al., The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation — I: Halo Gas Properties and the Role of SMBH Feedback
  • (abs, pdf) Sotillo-Ramos et al., The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
  • (abs, pdf) Pérez-González et al., CEERS Key Paper V: A triality on the nature of HST-dark galaxies
  • (abs, pdf) Chen et al., Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
  • (abs, pdf) Izquierdo et al., Global high-order numerical schemes for the time evolution of the general relativistic radiation magneto-hydrodynamics equations

19 Oct 2022

  • (abs, pdf) Byrne et al., Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
  • (abs, pdf) Neyer & Wolcott-Green, HI-shielding of ${\rm H_2}$ in UV-irradiated protogalaxies: suppression of the photodissociation rate
  • (abs, pdf) Jiménez et al., The physical drivers of gas turbulence in simulated disc galaxies
  • (abs, pdf) Clark et al., pynucastro: A Python Library for Nuclear Astrophysics

11 Oct 2022

  • (abs, pdf) Karunakaran et al., The Quenched Satellite Population Around Milky Way Analogs
  • (abs, pdf) Kaasinen et al., To See or Not to See a $z\sim13$ Galaxy? That is the Question
  • (abs, pdf) Laufman et al., On the triggering of extreme starburst events in low-metallicity galaxies: a deep search for companions of Green Peas
  • (abs, pdf) Gent et al., The small-scale dynamo in a multiphase supernova-driven medium
  • (abs, pdf) Torniamenti, A novel generative method for star clusters from hydro-dynamical simulations

07 Oct 2022

  • (abs, pdf) Li et al., The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
  • (abs, pdf) Rantala et al., BIFROST: simulating compact subsystems in star clusters using a hierarchical fourth-order forward symplectic integrator code
  • (abs, pdf) Wu et al., Demographics of z ~ 6 Quasars in the Black Hole Mass-Luminosity Plane
  • (abs, pdf) Menon et al., Outflows Driven by Direct and Reprocessed Radiation Pressure in Massive Star Clusters