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An Empirically Calibrated [C II] Luminosity-Halo Mass Relation for Line Intensity Mapping
Millimeter-wave line intensity mapping aims to observe the high-redshift universe through the 158 $μ$m fine-structure line of [C II], the brightest far-infrared line of star-forming galaxies. Whether a [C II] experiment at $z>4$ measures the clustering of large-scale structure, which carries rich co
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