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We give an overview of complementarity and synergy in cosmology between theSquare Kilometre Array and future survey projects in other wavelengths. In theSKA era, precision cosmology will be limited by systematic errors and cosmicvariance, rather than statistical errors. However, combining and/orcross-correlating multi-wavelength data, from the SKA to the cosmic microwavebackground, optical/infrared and X-ray, substantially reduce these limitingfactors. In this chapter, we summarize future survey projects and showhighlights of complementarity and synergy, which can be very powerful to probemajor cosmological problems such as dark energy, modified gravity andprimordial non-Gaussianity.

Overview of Complementarity and Synergy with Other Wavelengths in Cosmology in the SKA era