Garrelt Mellema, León Koopmans, Hemant Shukla, Kanan K. Datta, Andrei Mesinger, Suman Majumdar, on behalf of the CD/EoR Science Working Group
Published 2015-01-17Version 1
We provide an overview of 21cm tomography of the Cosmic Dawn and Epoch of Reionization as possible with SKA-Low. We show why tomography is essential for studying CD/EoR and present the scales which can be imaged at different frequencies for the different phases of SKA- Low. Next we discuss the different ways in which tomographic data can be analyzed. We end with an overview of science questions which can only be answered by tomography, ranging from the characterization of individual objects to understanding the global processes shaping the Universe during the CD/EoR
Comments: 14 pages, 3 figures. Accepted for publication in the SKA Science Book 'Advancing Astrophysics with the Square Kilometre Array', to appear in 2015. PoS(AASKA14)010
Constraining the Astrophysics of the Cosmic Dawn and the Epoch of Reionization with the SKA
Reionization and Cosmic Dawn: theory and simulations
Emulating the Global 21-cm Signal from Cosmic Dawn and Reionization
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