Tag Archives: 21cm

06 Aug 2021

  • (abs, pdf) Tsukui & Iguchi, Spiral morphology in an intensely star-forming disk galaxy more than 12 billion years ago
  • (abs, pdf) Webb & Bovy, Variation in the Stellar Mass Function Along Stellar Streams
  • (abs, pdf) The HERA Collaboration et al., First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
  • (abs, pdf) Yunis et al., Self-Interacting Dark Matter in Cosmology: accurate numerical implementation and observational constraints
  • (abs, pdf) Rashkovetskyi et al., Small-scale Clumping at Recombination and the Hubble Tension

25 Jun 2021

  • (abs, pdf) Tamfal et al., The Dawn of Disk Formation in a Milky Way-sized Galaxy: Thin Stellar Disks at $z > 4$
  • (abs, pdf) Higgs & McConnachie, Solo dwarfs IV: Comparing and contrasting satellite and isolated dwarf galaxies in the Local Group
  • (abs, pdf) Gómez et al., Halo Merger Tree Comparison: Impact on Galaxy Formation Models
  • (abs, pdf) Horowitz et al., HyPhy: Deep Generative Conditional Posterior Mapping of Hydrodynamical Physics
  • (abs, pdf) Washinoue & Suzuki, Coronal Properties of Low-mass Population III Stars and the Radiative Feedback in the Early Universe
  • (abs, pdf) Erika et al., Hoyle-Lyttleton accretion on to black hole accretion disks with super-Eddington luminosity for dusty gas
  • (abs, pdf) Reis et al., Shot noise and scatter in the star formation efficiency as a source of 21-cm fluctuations
  • (abs, pdf) Matteucci, Modelling the chemical evolution of the Milky Way

10-14 May 2021

  • (abs, pdf) Allevato et al., Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
  • (abs, pdf) Sadanari et al., Magnetohydrodynamic effect on first star formation: prestellar core collapse and protostar formation
  • (abs, pdf) Pagano & Liu, Lyman Alpha Emitters and the 21cm Power Spectrum as Probes of Density-Ionization Correlation in the Epoch of Reionization
  • (abs, pdf) Carlsten et al., ELVES I: Structures of Dwarf Satellites of MW-like Galaxies; Morphology, Scaling Relations, and Intrinsic Shapes
  • (abs, pdf) Carlsten et al., ELVES II: GCs and Nuclear Star Clusters of Dwarf Galaxies; The Importance of Environment
  • (abs, pdf) Arentsen et al., The Pristine Inner Galaxy Survey (PIGS) III: carbon-enhanced metal-poor stars in the bulge
  • (abs, pdf) Das et al., Effect of mass loss due to stellar winds on the formation of supermassive black hole seeds in dense nuclear star clusters
  • (abs, pdf) Wibking & Krumholz, The global structure of magnetic fields and gas in simulated Milky Way-analogue galaxies
  • (abs, pdf) Grand et al., Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
  • (abs, pdf) Placco et al., SPLUSJ210428.01-004934.2: An Ultra Metal-Poor Star Identified from Narrowband Photometry
  • (abs, pdf) Greene et al., A Search for Wandering Black Holes in the Milky Way with Gaia and DECaLS
  • (abs, pdf) Sahlén & Zackrisson, Galaxy population constraints on cosmology and star formation in the early Universe
  • (abs, pdf) Gelli et al., Dwarf satellites of high-z Lyman Break Galaxies: a free lunch for JWST
  • (abs, pdf) Gilman et al., Strong lensing signatures of self-interacting dark matter in low-mass halos
  • (abs, pdf) Chowdhury et al., On the Random Motion of Nuclear Objects in a Fuzzy Dark Matter Halo

15 Apr 2021

  • (abs, pdf) Fahrion et al., Diversity of nuclear star cluster formation mechanisms revealed by their star formation histories
  • (abs, pdf) Wang et al., SpaceHub: A high-performance gravity integration toolkit for few-body problems in astrophysics
  • (abs, pdf) Breysse et al., Mapping the Universe in HD
  • (abs, pdf) Juneau et al., Jupyter-Enabled Astrophysical Analysis for Researchers and Students
  • (abs, pdf) Yang et al., A New Fast Monte Carlo Code for Solving Radiative Transfer Equations based on Neumann Solution
  • (abs, pdf) Dawoodbhoy et al., Core-Envelope Haloes in Scalar Field Dark Matter with Repulsive Self-Interaction: Fluid Dynamics Beyond the de Broglie Wavelength