The project pushed the envelope by integrating optical and infrared data from the KiDS and VIKING surveys, respectively, for the first time in a cosmic shear measurement. This was done to improve photometric redshifts, select galaxies at higher redshift (i.e. earlier cosmic times), and push down the statistical uncertainties. This was complemented by a coherent effort to also increase our knowledge of the most important systematic errors, again with a particular focus on the redshift calibration. Final results from KiDS+VIKING (to be published before the end of 2024) will be 30-40% more constraining than the best current results thanks to the work of the COSMIC-LITMUS team. If the results don't change significantly, the odds for the standard model being correct will be vanishingly small by that point.
At the same time, we increased our efforts within the Euclid and LSST consortia, applying the techniques that have been pioneered on KiDS+VIKING on these new data sets as they come online. No matter what the final KiDS+VIKING analysis will tell us about the S8 tension in the end, the lessons learned there will be invaluable to make sure that Euclid and LSST meet their primary scientific goal of determining the physical nature of dark energy.