Speaker
Carlo Burigana
(Istituto Nazionale di Astrofisica (INAF))
Description
The synergy between current and future cosmic microwave background (CMB) projects and the extreme sensitivity and resolution of the Square Kilometre Array (SKA) will be crucial for a wide set of themes relevant for cosmology and astrophysics at different cosmic epochs, including cosmological parameter estimation, integrated Sachs-Wolfe effect and constraints on dark energy, primordial non-Gaussianity and magnetic fields, CMB spectrum and cosmological reionization. I discuss the instrumental requirements and the observational/data analysis approaches relevant for performing these scientific investigations.
Primary author
Carlo Burigana
(Istituto Nazionale di Astrofisica (INAF))
