# Recovering the HII region size statistics from 21-cm tomography

**Authors:** Koki Kakiichi, Suman Majumdar, Garrelt Mellema, Benedetta Ciardi, Keri, L. Dixon, Ilian T. Iliev, Vibor Jelic, Leon V. E. Koopmans, Saleem Zaroubi,, Philipp Busch

arXiv: 1702.02520 · 2017-10-23

## TL;DR

This paper presents granulometry, a new mathematical technique to extract the size distribution of HII regions from 21-cm tomography data, enabling better understanding of reionization with current and future radio telescopes.

## Contribution

The paper introduces granulometry as a novel, mathematically grounded method for recovering HII region size statistics from 21-cm tomography data.

## Key findings

- Granulometry can recover HII region size distribution at moderate SNR (~3).
- The method is effective with wide-field imaging and interferometric mosaicking.
- Observational requirements include specific angular resolution and field-of-view.

## Abstract

We introduce a novel technique, called "granulometry", to characterize and recover the mean size and the size distribution of HII regions from 21-cm tomography. The technique is easy to implement, but places the previously not very well defined concept of morphology on a firm mathematical foundation. The size distribution of the cold spots in 21-cm tomography can be used as a direct tracer of the underlying probability distribution of HII region sizes. We explore the capability of the method using large-scale reionization simulations and mock observational data cubes while considering capabilities of SKA1-low and a future extension to SKA2. We show that the technique allows the recovery of the HII region size distribution with a moderate signal-to-noise ratio from wide-field imaging ($\rm SNR\lesssim3$), for which the statistical uncertainty is sample variance dominated. We address the observational requirements on the angular resolution, the field-of-view, and the thermal noise limit for a successful measurement. To achieve a full scientific return from 21-cm tomography and to exploit a synergy with 21-cm power spectra, we suggest an observing strategy using wide-field imaging (several tens of square degrees) by an interferometric mosaicking/multi-beam observation with additional intermediate baselines (~2-4 km).

## Full text

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## Figures

32 figures with captions in the complete paper: https://tomesphere.com/paper/1702.02520/full.md

## References

73 references — full list in the complete paper: https://tomesphere.com/paper/1702.02520/full.md

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Source: https://tomesphere.com/paper/1702.02520