Category Archives: astro-ph
Here are the papers from astro-ph that I find interesting. I tend to update daily, so if there is a day missing, I probably didn’t find any papers relevant to our group.
12 Jan 2021
- (abs, pdf) Wang et al., A Luminous Quasar at Redshift 7.642
- (abs, pdf) Barreto-Mota et al., Magnetic Field Orientation in Self-Gravitating Turbulent Molecular Clouds
- (abs, pdf) Falck et al., Indra: a Public Computationally-Accessible Suite of Cosmological $N$-body Simulations
- (abs, pdf) Kapahtia et al., Prospects of constraining reionization model parameters using … Continue Reading ››
11 Jan 2021
08 Jan 2021
- (abs, pdf) Villaume et al., Spatially Resolved Stellar Spectroscopy of the Ultra-diffuse Galaxy Dragonfly 44. III. Evidence for an Unexpected Star-Formation History
- (abs, pdf) McKenzie & Bekki, Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics
- (abs, pdf) Orkney et al., EDGE: Two routes to dark … Continue Reading ››
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 … Continue Reading ››
06 Jan 2021
- (abs, pdf) Worseck et al., Dating individual quasars with the HeII proximity effect
- (abs, pdf) Izumi et al., Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) XII. Extended [C II] Structure (Merger or Outflow) in a z = 6.72 Red Quasar
- (abs, pdf) Morales et al., The Evolution of the Lyman-Alpha Luminosity … Continue Reading ››
05 Jan 2021
- (abs, pdf) Zubovas & King, High-redshift SMBHs can grow from stellar-mass seeds via chaotic accretion
- (abs, pdf) Yang et al., The prospects for observing [OIII] 52 micron emission from galaxies during the Epoch of Reionization
- (abs, pdf) Ramsøy et al., Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments