Tag Archives: 21cm

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

16 Mar 2021

  • (abs, pdf) Minniti et al., Discovery of new globular clusters in the Sagittarius dwarf galaxy
  • (abs, pdf) Ghara et al., Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
  • (abs, pdf) Mackey et al., PION: Simulating bow shocks and circumstellar nebulae
  • (abs, pdf) Bland-Hawthorn et al., Quantum memories and the double-slit experiment: implications for astronomical interferometry
  • (abs, pdf) Woosley & Heger, The Pair-Instability Mass Gap for Black Holes
  • (abs, pdf) Efstathiou et al., A hyperluminous obscured quasar at a redshift of z ~ 4.3

07 Jan 2021

  • (abs, pdf) Grisdale et al., Predicting the Observability of Population III Stars with ELT-HARMONI via the Helium $1640{\rm\AA}$ emission line
  • (abs, pdf) Reis et al., The subtlety of Ly-a photons: changing the expected range of the 21-cm signal
  • (abs, pdf) May & Springel, Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics

30 Nov 2020

  • (abs, pdf) Font et al., Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?
  • (abs, pdf) Dalal et al., Don't cross the streams: caustics from Fuzzy Dark Matter
  • (abs, pdf) Binggeli et al., A puzzling non-detection of [O III] and [C II] from a $z \approx 7.7$ galaxy observed with ALMA
  • (abs, pdf) Santos-Santos et al., Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
  • (abs, pdf) Tanaka & Hasegawa, Modelling Population III stars for semi-numerical simulations
  • (abs, pdf) Huang et al., Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
  • (abs, pdf) Schneider et al., A halo model approach for the 21-cm power spectrum at cosmic dawn

10 Nov 2020

  • (abs, pdf) Hammer et al., MOSAIC on the ELT: high-multiplex spectroscopy to unravel the physics of stars and galaxies from the dark ages to the present-day
  • (abs, pdf) Perez et al., Void Probability Function of Simulated Surveys of high-redshift Lyman-Alpha Emitters
  • (abs, pdf) Ross et al., Redshift-space distortions in simulations of the 21-cm signal from the cosmic dawn
  • (abs, pdf) Gangolli et al., Constraining Reionization in Progress at z=5.7 with Lyman-$\alpha$ Emitters: Voids, Peaks, and Cosmic Variance
  • (abs, pdf) Ahn & Shapiro, Cosmic Reionization May Still Have Started Early and Ended Late: Confronting Early Onset with CMB Anisotropy and 21 cm Global Signals