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Tomography of cosmic reionization and large-scale structure of the Universe at redshifts 3 – 8 (C03)

Subject Area Astrophysics and Astronomy
Term since 2023
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 500700252
 
Through line intensity mapping (LIM) of the habitats of massive stars in galaxies on Mpc to tens of Mpc scales with FYST/CCAT-prime, it will become possible to constrain the distribution of hydrogen-ionising photons during cosmic reionisation through the clustering of the galaxies that emit them. This will yield a three-dimensional tomographic map of the expected progression of cosmic reionisation with time in different environments in the early universe, when massive stars first formed.
DFG Programme Collaborative Research Centres
Applicant Institution Universität zu Köln
 
 

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