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

• Published in: Astronomy and astrophysics (Berlin) 2021-09, Vol.653, p.A58
• Main Authors: Gorce, A., Hutter, A., Pritchard, J. R.
• Format: Article
• Language: English
• Subjects: Astrophysics; Brightness temperature; Differential thermal analysis; Galaxies; Ionization; Morphology; Physics; Radio telescopes; Red shift; Sample variance; Topology; Variance
• ISSN: 0004-6361; 1432-0746; 1432-0756
• DOI: 10.1051/0004-6361/202140515

Intensity mapping of the 21 cm 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, 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, which we refer to as the local variance, σ loc , that describes the distribution of the mean differential 21 cm 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 gain insight into the ionising properties of early galaxies.