Introducing SAGUARO -- Simulating IGM Evolution and Environments At High Resolution: Setup and First Results
astro-ph.CO, astro-ph.GA
Submitted: 2026-03-26
Updated: 2026-09-24
Terminology
Sources
- Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Ly$\alpha$ forest data
- Evidence of patchy hydrogen reionization from an extreme Ly$\alpha$ trough below redshift six
- Large Lyman-alpha opacity fluctuations and low CMB tau in models of late reionization with large islands of neutral hydrogen extending to z<5.5
- Constraining the second half of reionization with the Lyman-$\beta$ forest
- Hydrogen reionisation ends by $z=5.3$: Lyman-$\alpha$ optical depth measured by the XQR-30 sample
- Chasing the Tail of Cosmic Reionization with Dark Gap Statistics in the Ly$\alpha$ Forest over $5 < z < 6$
- (Nearly) Model-Independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at $z\sim 5-7$ Using Dark Pixel Fractions in Ly$\alpha$ and Ly$\beta$ Forests
- Damping wing absorption associated with a giant Ly$\alpha$ trough at $z < 6$: direct evidence for late-ending reionization
- Damping Wing-Like Features in the Stacked Ly$\alpha$ Forest: Potential Neutral Hydrogen Islands at $z<6$
- A Significantly Neutral Intergalactic Medium Around the Luminous z=7 Quasar J0252-0503
- JWST/NIRSpec Observations of Ly$\alpha$ Emission in Star Forming Galaxies at $6.5\lesssim z\lesssim13$
- Multivariate Predictors of LyC Escape II: Predicting LyC Escape Fractions for High-Redshift Galaxies
- Galaxies in the Epoch of Reionization Are All Bark and No Bite -- Plenty of Ionizing Photons, Low Escape Fractions
- Chronicling the reionization history at $6\lesssim z \lesssim 7$ with emergent quasar damping wings
- Precisely Measuring the Cosmic Reionization History from IGM Damping Wings Towards Quasars
- Beacons into the Cosmic Dark Ages: Boosted transmission of Ly$\alpha$ from UV bright galaxies at $z \gtrsim 7$
- JWST Measurements of Neutral Hydrogen Fractions and Ionized Bubble Sizes at $z=7-12$ Obtained with Ly$\alpha$ Damping Wing Absorptions in 27 Bright Continuum Galaxies
- JADES NIRSpec Spectroscopy of GN-z11: Lyman-$\alpha$ emission and possible enhanced nitrogen abundance in a $z=10.60$ luminous galaxy
- EPOCHS Paper II: The Ultraviolet Luminosity Function from $7.5<z<13.5$ using 180 square arcminutes of deep, blank-fields from the PEARLS Survey and Public JWST data
- JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$
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