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We combine available constraints on the local CII 158 $\mu$m line luminosityfunction from galaxy observations (Hemmati et al. 2017), with the evolution ofthe star-formation rate density and the recent CII intensity mappingmeasurement in Pullen et al. (2018, assuming detection), to derive theevolution of the CII luminosity - halo mass relation over $z \sim 0-6$. Wedevelop convenient fitting forms for the evolution of the CII luminosity - halomass relation, and forecast constraints on the CII intensity mapping powerspectrum and its associated uncertainty across redshifts. We predict thesensitivities to detect the power spectrum for upcoming PIXIE-, STARFIRE-,EXCLAIM-, CONCERTO-, TIME- and CCAT-p-like surveys, as well as possible futureintensity mapping observations with the ALMA facility.

Constraining the evolution of CII intensity through the end stages of reionization