27 Jun – 01 Jul 2022

  • (abs, pdf) Baier-Soto et al., A tentative $\sim$1000 km s$^{-1}$ offset between the [CII] 158 $\mu$m and Ly$\alpha$ line emission in a star-forming galaxy at $z = 7.2$
  • (abs, pdf) Cadiou et al., Stellar angular momentum can be controlled from cosmological initial conditions
  • (abs, pdf) Gough & Uhlemann, Making (dark matter) waves: Untangling wave interference for multi-streaming dark matter
  • (abs, pdf) Yung et al., Semi-analytic forecasts for JWST — VI. Simulated lightcones and galaxy clustering predictions
  • (abs, pdf) Stefanon et al., Deep Spitzer/IRAC Data for z~10 galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ~500 Myr of Cosmic Time
  • (abs, pdf) Calura et al., Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars
  • (abs, pdf) Lombardo et al., Chemical Evolution of R-process Elements in Stars (CERES). I. Stellar parameters and chemical abundances from Na to Zr
  • (abs, pdf) Briel et al., Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
  • (abs, pdf) Mas-Ribas et al., LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
  • (abs, pdf) Sun et al., LIMFAST. II. Line Intensity Mapping as a Probe of High-Redshift Galaxy Formation
  • (abs, pdf) Menon et al., Infrared Radiation Feedback Does Not Regulate Star Cluster Formation or Drive Winds
  • (abs, pdf) Toyouchi et al., Radiative feedback on supermassive star formation: the massive end of the Population III initial mass function
  • (abs, pdf) Bernal & Kovetz, Line-Intensity Mapping: Theory Review

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