- (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*

# Tag Archives: 21cm

# 18 Mar 2021

- (abs, pdf) Ma et al.,
*Investigating X-ray sources during the epoch of reionization with the 21 cm signal* - (abs, pdf) Gan et al.,
*SeeingGAN: Galactic image deblurring with deep learning for better morphological classification of galaxies* - (abs, pdf) Baltimore et al.,
*Should the Endless Frontier of Federal Science be Expanded?*

# 17 Mar 2021

- (abs, pdf) Trujillo-Gomez et al.,
*The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters* - (abs, pdf) Burns et al.,
*A Lunar Farside Low Radio Frequency Array for Dark Ages 21-cm Cosmology* - (abs, pdf) Efstathiou,
*To H0 or not to H0?* - (abs, pdf) Guidetti et al.,
*dNNsolve: an efficient NN-based PDE solver*

# 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*

# 16 Feb 2021

# 19 Jan 2021

# 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*

# 15 Dec 2020

# 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*