We produce simulations of the atomic C II line emission in large sky fields in order to determine the current and future prospects for mapping this line during the high-redshift epoch of reionization. We calculate the C II line intensity, redshift evolution, and spatial fluctuations using observational relations between C II emission and the galaxy star formation rate over the frequency range 200-300 GHz. We estimate an averaged intensity of
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Silva et al. (2015) studied this question.
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