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The Renaissance Simulations Vault
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The Renaissance Simulations Vault
  • Project Information
    • Motivation
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  • Background
    • Physics Background
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  • Data
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    • JWST Predictions
  • Project Info
  • Results
  • Published Works
  • Scaling Relations for Galaxies Prior to Reionization
  • Spatially Extended 21 cm Signal from Strongly Clustered Uv and X-Ray Sources in the Early Universe
  • Probing the Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations
  • Late Pop III Star Formation During the Epoch of Reionization: Results from the Renaissance Simulations
  • X-Ray Background at High Redshifts from Pop III Remnants: Results from Pop III Star Formation Rates in the Renaissance Simulations
  • Population III Stars and Remnants in High Redshift Galaxies
  • Galaxy Properties and UV Escape Fractions during the Epoch of Reionization: Results from the Renaissance Simulations
  • Heating the Intergalactic Medium by X-Rays from Population III Binaries in High-redhsift Galaxies
  • First light: exploring the spectra of high-redshift galaxies in the Renaissance Simulations
  • First light – II. Emission line extinction, population III stars, and X-ray binaries
  • Fully Coupled Simulation of Cosmic Reionization. III. Stochastic Early Reionization by the Smallest Galaxies
  • The growth of black holes from Population III remnants in the Renaissance simulations
  • Simulating the Cosmic Dawn With Enzo
  • Formation of massive black holes in rapidly growing pre-galactic gas clouds
  • The emergence of the first star-free atomic cooling haloes in the Universe
  • Massive Star Formation in Metal-Enriched Haloes at High Redshift
  • Some First Stars Were Red: Detecting Signatures of Massive Population III Formation through Long-term Stochastic Color Variations
  • How long do high-redshift massive black hole seeds remain outliers in black hole vs. host galaxy relations?
  • No Tension: JWST Galaxies at z > 10 Consistent with Cosmological Simulations
  • Beyond the Goldilocks Zone: Identifying Critical Features in Massive Black Hole Formation
  • Explore the Data
  • Beyond No Tension: JWST z > 10 Galaxies Push Simulations to the Limit
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