Explore the Early Universe

Navigate Cosmological Simulations

Search for the First Generation of Stars

Predict James Webb Space Telescope Observations

Welcome to the Universe

The James Webb Space Telescope (JWST), launched in December 2021, has delivered a tidal wave of observations of the early universe. These observations are a critical step toward understanding the birth and evolution of the first generations of stars.

The Renaissance Simulations trace the evolution of early galaxies  until they reach epochs observable by JWST. By directly comparing simulation results with Webb’s data, researchers can test how well their theoretical models agree with observations of the early universe. Together, JWST and the Renaissance Simulations provide an unprecedented opportunity to build the first complete history of early star formation.

All Renaissance Simulation datasets used in this work are available for download directly through this website. Making the data openly accessible allows researchers, students, and the broader community to explore the formation and evolution of the first galaxies alongside JWST’s observations.

Renaissance Simulations

The Renaissance Simulations are high resolution, low mass (less than 107 M⊙), high-redshift (z > 10) zoom in simulations that model the first galaxies. They were run using adaptive mesh refinement code ENZO and consisted of three main regions: the Normal, Void, and Rarepeak. These regions respectively represent areas of normal, low, and high mass densities.

James Webb Space Telescope (JWST)

JWST has given humanity data of the early universe which has elevated our ability to study the Epoch of Reionization (z ≥ 6) and Cosmic High Noon (z = 2–6). The Renaissance Simulations are being compared against the highest redshift galaxies found by JWST Advanced Deep Extragalactic Survey (JADES) and the Cosmic Evolution Early Release (CEERS) surveys. Older objects in the universe can be seen in infrared light so these surveys are using JWST’s Near-Infrared Spectrograph (NIRSpec) and the Near-Infrared Camera (NIRCam) which operate over the wavelengths 0.6 – 5 µm.

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