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We present the science enabled by cross-correlations of the SKA1-LOW 21-cmEoR surveys with other line mapping programs. In particular, we identify andinvestigate potential synergies with planned programs, such as the lineintensity mapping of redshifted CO rotational lines, [CII] and Ly-$\alpha$emissions during reionization. We briefly describe how these tracers of thestar-formation rate at $z \sim 8$ can be modeled jointly before forecastingtheir auto- and cross-power spectra measurements with the nominal 21cm EoRsurvey. The use of multiple line tracers would be invaluable to validate andenrich our understanding of the EoR.

Synergy of CO/[CII]/Ly$\alpha$ Line Intensity Mapping with the SKA