Marika Asgari

The Kilo Degree Survey (KiDS) has collected all of its images which form the basis of its 5th and final data release (KiDS-Legacy). In this talk I will summarise the resulting cosmic shear analysis from KiDS-Legacy and detail the various systematic and consistency tests that we performed to ensure its robustness. We find that with our new analysis choices and extra data the tension in S8 with respect to CMB data from Planck-Legacy has reduced to less than 1 sigma (assuming a flat-LCDM model), rendering it insignificant. At the end of this talk, I will point to the remaining cosmological analyses that are expected to be released in the near future.