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The Reionization Parameter Space Consistent with the Thomson Optical Depth from Planck

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abstract

We study the reionization parameter space consistent with the current measurement of the Thomson optical depth using a new parametrization of the reionization history. The mass-weighted ionization fraction is specified in terms of the redshift midpoint, duration, and asymmetry shape parameters. We perform an MCMC analysis using conservative flat priors and physical constraints. Our analysis yields a redshift midpoint of $z_{50}=7.66\substack{+0.57-0.61}\text{(68%)}\substack{+1.26-1.02}\text{(95%)}$, and upper limits on the duration $\Delta_\text{z} < 7.5$ and asymmetry $A_\text{z}<5.3$ for $\tau = 0.054 \pm 0.007$. The reconstructed mass-weighted ionization fraction $x_\text{i}(z)$ is asymmetric, but early contributions to reionization are minor.

fields

astro-ph.CO 1

years

2026 1

verdicts

UNVERDICTED 1

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The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization

astro-ph.CO · 2026-05-18 · unverdicted · novelty 4.0

The Lumina simulation shows that explicit light-cone integrations produce a CMB optical depth 7% higher than volume-weighted ionization histories, with the excess accumulating near redshift 8 and mass-weighted estimates capturing most of the difference.

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  • The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization astro-ph.CO · 2026-05-18 · unverdicted · none · ref 35 · internal anchor

    The Lumina simulation shows that explicit light-cone integrations produce a CMB optical depth 7% higher than volume-weighted ionization histories, with the excess accumulating near redshift 8 and mass-weighted estimates capturing most of the difference.