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Cosmic Reionization On Computers: Biases and Uncertainties in the Measured Mean Free Path at the End Stage of Reionization
Published 2025-06-01“…Recent observations and analyses of absorption in quasar spectra suggest a rapid drop in the mean free path (MFP) at the late stage of reionization at $z\sim6$. We use the Cosmic Reionization on Computers simulation to examine potential biases in observed measurements of the MFP at the late stage of reionization, particularly in the presence of a quasar. …”
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Chasing the Beginning of Reionization in the JWST Era
Published 2025-01-01Subjects: “…Reionization…”
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Constraining Reionization with Lyα Damping-wing Absorption in Galaxy Spectra: A Machine Learning Model Based on Reionization Simulations
Published 2025-01-01Subjects: “…Reionization…”
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Central Concentration and Escape of Ionizing Photons in Galaxies at the Epoch of Reionization
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The Cosmic Microwave Background Optical Depth Constrains the Duration of Reionization
Published 2025-01-01Subjects: “…Reionization…”
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NuSTAR Observations of a Varying-flux Quasar in the Epoch of Reionization
Published 2025-01-01“…This brightening is one of the most extreme instances of statistically significant X-ray variability seen in the Epoch of Reionization. We discuss possible scenarios that could produce such rapid change, including X-ray emission from jets too faint at radio frequencies to be observed.…”
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Behavior of the Lyα Damping Wings as a Function of Reionization Topology
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Constraints on the Galaxy Formation Models during the Epoch of Reionization with High-redshift Observations
Published 2025-01-01Subjects: “…Reionization…”
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EPOCHS. XI. The Structure and Morphology of Galaxies in the Epoch of Reionization to z ∼ 12.5
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Revisiting the Intergalactic Medium around GRB 130606A and Constraints on the Epoch of Reionization
Published 2025-01-01Subjects: “…Reionization…”
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The Evolving Power Spectrum for the Light Cone Epoch of Reionization 21 cm Signal
Published 2025-01-01Subjects: “…Reionization…”
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LIMFAST. III. Timing Cosmic Reionization with the 21 cm and Near-infrared Backgrounds
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Optimal, fast, and robust inference of reionization-era cosmology with the 21cmPIE-INN
Published 2025-04-01“…Modern machine learning will allow for simulation-based inference from reionization-era 21cm observations at the Square Kilometre Array. …”
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Nature of High Equivalent Width Emitters in the Epoch of Reionization Revealed by JWST Medium-band Imaging
Published 2025-01-01“…Extreme emission line galaxies (EELGs) at high redshifts are considered key contributors to cosmic reionization at z > 6 due to their higher ionization efficiencies. …”
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Direct Evidence for Active Galactic Nuclei Feedback from Fast Molecular Outflows in Reionization-era Quasars
Published 2025-01-01“…This represents the first survey for molecular winds in reionization-era quasars, and we detect unambiguous outflows in 8/11 (73%) of the quasars. …”
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Three Quenched, Faint Dwarf Galaxies in the Direction of NGC 300: New Probes of Reionization and Internal Feedback
Published 2024-01-01“…The discovery of three dwarf galaxies in isolated or low-density environments offers an opportunity to study the varying effects of ram-pressure stripping, reionization, and internal feedback in influencing the star formation history of the faintest stellar systems.…”
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First Measurements of Black Hole Accretion and Radio-jet Timescales in a Young Quasar at the Edge of Reionization
Published 2025-01-01“…We present the first study dedicated to measuring the timescales for black hole accretion and jet launching in a quasar at the edge of reionization, PSO J352.4034–15.3373 at z = 5.832 ± 0.001. …”
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The Impact of Stellar Initial Mass Function on the Epoch of Reionization: Insights from Semi-Analytic Galaxy Modeling
Published 2025-04-01Subjects: Get full text
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Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations: Methods and Parameter Exploration
Published 2022-01-01“…We post-process a simulation from the Cosmic Reionization on Computers project, integrating an ordinary differential equation for the evolution of the dust-to-gas ratio along pathlines in the simulation sampled with a tracer particle technique. …”
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