869 citations · 7.6k across the 94 of their papers we have counts for
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Why does the Milky Way have a metallicity floor?
Britton D. Smith, Brian W. O'Shea, Sadegh Khochfar +3
The prevalence of light element enhancement in the most metal-poor stars is potentially an indication that the Milky Way has a metallicity floor for star formation around 10$…
Emulating Radiative Transfer with Artificial Neural Networks
Snigdaa S. Sethuram, Rachel K. Cochrane, Christopher C. Hayward +4
Forward-modeling observables from galaxy simulations enables direct comparisons between theory and observations. To generate synthetic spectral energy distributions (SEDs) that inc…
Neutron Star Mergers and their Impact on Second Generation Star Formation in the Early Universe
Danielle Skinner, John H. Wise
The exact evolution of elements in the universe, from primordial to heavier elements produced via the r-process, is still under scrutiny. The supernova deaths of the very first sta…
The Role of Radiation and Halo Mergers in Pop III Star Formation
Lilia Correa Magnus, Britton D. Smith, Sadegh Khochfar +4
We present a study of the co-evolution of a population of primordial star-forming minihalos at Cosmic Dawn. In this study, we highlight the influence of individual Population III s…
No Tension: JWST Galaxies at Consistent with Cosmological Simulations
Joe McCaffrey, Samantha Hardin, John Wise +1
Recent observations by JWST have uncovered galaxies in the very early universe via the JADES and CEERS surveys. These galaxies have been measured to have very high stellar masses w…
EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely-Metal Poor Galaxies
Yi Xu, Masami Ouchi, Yuki Isobe +49
We present demography of the dynamics and gas-mass fraction of 33 extremely metal-poor galaxies (EMPGs) with metallicities of and low stellar masses of $10^4-…