Imaging the 21-cm Signal from the Cosmic Dawn & Epoch of Reionization and the Connection with the Global Signal
Satadru Bag, Michele Bianco, Samir Choudhuri, Saswata Dasgupta, Abhirup Datta, Kanan K. Datta, Ivelin Georgiev, Sambit K. Giri, Ian Hothi, Akanksha Kapahtia, Suman Majumdar, Garrelt Mellema, Arnab Mishra, Samit Kumar Pal, Feiyu Zhao
astro-ph.CO
Submitted: 2026-06-23
Comments: Published in Advancing Astrophysics with the SKA II (AASKAII), 2026 (arXiv:2606.20366). Report-no:AASKAII/Bag01
License: http://creativecommons.org/licenses/by-nc-sa/4.0/
The gist: The original baseline design for SKA-Low was motivated by the ability to produce tomographic images of the redshifted 21-cm signal, thus allowing the research field to move beyond the simple
Terminology
Abstract
The original baseline design for SKA-Low was motivated by the ability to produce tomographic images of the redshifted 21-cm signal, thus allowing the research field to move beyond the simple statistic of the power spectrum. In this chapter we review the imaging capabilities of SKA-Low, the wide variety of methods proposed for quantatively analysing image data, as well as the connection with the global 21-cm signal.
Sources
- Exploring the Geometry, Topology and Morphology of Large Scale Structure using Minkowski Functionals
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