Tag Archives: Dust

03 Nov 2022

  • (abs, pdf) Jones et al., Gas-rich, field ultra-diffuse galaxies host few globular clusters
  • (abs, pdf) Hahn et al., ${\rm S{\scriptsize IM}BIG}$: A Forward Modeling Approach To Analyzing Galaxy Clustering
  • (abs, pdf) Capelo et al., Black hole-galaxy co-evolution and the role of feedback
  • (abs, pdf) da Cunha, The dust properties of star-forming galaxies in the first billion years
  • (abs, pdf) Saldana-Lopez et al., The VANDELS survey: the ionizing properties of star-forming galaxies at $3 \leq z \leq 5$ using deep rest-frame ultraviolet spectroscopy

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 isolated and merging galaxies with an explicit, multiphase ISM
  • (abs, pdf) Hu et al., Long-term evolution of supercritical black hole accretion with outflows: a subgrid feedback model for cosmological simulations
  • (abs, pdf) Flury et al., The Low-Redshift Lyman Continuum Survey II: New Insights into LyC Diagnostics
  • (abs, pdf) Viero et al., The Early Universe was Dust-Rich and Extremely Hot

03 Aug 2021

  • (abs, pdf) Imara et al., Touching the Stars: Using High-Resolution 3D Printing to Visualize Stellar Nurseries
  • (abs, pdf) Nuñez et al., Empirical Constraints on Core Collapse Supernova Yields using Very Metal Poor Damped Lyman Alpha Absorbers
  • (abs, pdf) Vijayan et al., First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
  • (abs, pdf) Vericel et al., Dust growth, fragmentation and self-induced dust traps in PHANTOM
  • (abs, pdf) Katz et al., The Nature of High ${\rm [OIII]}_{\rm 88\mu m}$/${\rm [CII]}_{\rm 158\mu m}$ Galaxies in the Epoch of Reionization: Low Carbon Abundance and a Top-Heavy IMF?