- (abs, pdf) Zana et al., Enhanced star formation in $z\sim6$ quasar companions
- (abs, pdf) Lewis et al., DUSTiER (DUST in the Epoch of Reionization): dusty galaxies in cosmological radiation-hydrodynamical simulations of the Epoch of Reionization with RAMSES-CUDATON
- (abs, pdf) Ma et al., A CRASH simulation of the contribution of binary stars … Continue Reading ››
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.
08 Apr 2022
07 Apr 2022
06 Apr 2022
05 Apr 2022
- (abs, pdf) Sameie et al., Formation of proto-globular cluster candidates in cosmological simulations of dwarf galaxies at $z>4$
- (abs, pdf) Andika et al., Staring at the Shadows of Archaic Galaxies: Damped Ly$\alpha$ and Metal Absorbers toward a Young $z \sim 6$ Weak-line Quasar
- (abs, pdf) Biscoveanu et al., … Continue Reading ››
04 Apr 2022
01 Apr 2022
- (abs, pdf) Lehmer et al., Elevated Hot Gas and High-Mass X-ray Binary Emission in Low Metallicity Galaxies: Implications for Nebular Ionization and Intergalactic Medium Heating in the Early Universe
- (abs, pdf) Rodriguez et al., Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky … Continue Reading ››
31 Mar 2022
30 Mar 2022
- (abs, pdf) Spilker et al., Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo
- (abs, pdf) Bouwens et al., z~2-9 Galaxies magnified by the Hubble Frontier Field Clusters I: Source Selection and Surface Density-Magnification Constraints from >2500 galaxies
- (abs, pdf) Sivasankaran et al., Simulations of black hole fueling in … Continue Reading ››
29 Mar 2022
- (abs, pdf) Spinoso et al., Multi-flavour SMBH seeding and evolution in cosmological environments
- (abs, pdf) Braspenning et al., Sensitivity of non-radiative cloud-wind interactions to the hydrodynamics solver
- (abs, pdf) Adams et al., Axion Dark Matter
- (abs, pdf) Antypas et al., New Horizons: Scalar and Vector Ultralight Dark Matter