I will review the theoretical challenges to model the HI content in the post-reionization universe. I will address both astrophysical and cosmological questions that can be addressed by exploiting the 21 cm signal with SKA.
I will discuss the cosmological constraints from the combination and cross-correlation of radio, optical, and microwave cosmological observations in order to obtain precise measurements of perturbations on large scales.
Specifically I will show that a conservative combination of an SKAO-MID HI intensity mapping survey with the galaxy clustering from two photometric galaxy surveys (Euclid-...
The new generation radio telescopes, such as the Square Kilometre Array (SKA), are expected to reach sufficient sensitivity and resolution to provide large number densities of resolved faint sources, and therefore to open weak gravitational lensing observations to the radio band. In this talk I will present RadioLensfit, an open-source tool for an efficient and fast galaxy shape measurement...