Using the sample variance of 21cm maps as a tracer of the ionisation topology

TL;DR

This paper introduces a new local variance statistic for 21cm intensity maps that effectively traces the reionisation history and ionisation morphology, aiding in understanding early universe galaxy properties.

Contribution

The paper presents a novel local variance measure that leverages observational sample variance to analyze 21cm maps, providing new insights into reionisation and galaxy ionising properties.

Findings

Local variance traces reionisation history.

It helps constrain the midpoint of reionisation.

Provides insights into ionising properties of early galaxies.

Abstract

Intensity mapping of the 21cm signal of neutral hydrogen will yield exciting insights into the Epoch of Reionisation and the nature of the first galaxies. However, the large amount of data that will be generated by the next generation of radio telescopes, such as the Square Kilometre Array (SKA), as well as the numerous observational obstacles to overcome, require analysis techniques tuned to extract the reionisation history and morphology. In this context, we introduce a one-point statistic, to which we refer as the local variance, $\sigma_\mathrm{loc}$, that describes the distribution of the mean differential 21cm brightness temperatures measured in two-dimensional maps along the frequency direction of a light-cone. The local variance takes advantage of what is usually considered an observational bias, the sample variance. We find the redshift-evolution of the local variance to not only probe the reionisation history of the observed patches of the sky, but also trace the ionisation morphology. This estimator provides a promising tool to constrain the midpoint of reionisation as well as gaining insight into the ionising properties of early galaxies.