Cake Talk by Ian Hothi from Imperial College London
With current and upcoming radio interferometers, there is a need to find the optimal foreground removal technique. I will first present a comparison of these techniques in the context of LOFAR. There is growing evidence that Reionization is a more extended process than previously thought, with a potential of Reionization concluding by a redshift of 5.3 Next, I will present potential synergies between radio telescopes and upcoming surveys such as JWST and Euclid, and how this synergy can be used to better understand the end of Reionization. These cross-correlations not only have the potential for foreground mitigation but also enhanced constraints of reionization and the state of the IGM at the end of Reionization.