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Cold Gas in High-z Galaxies: The Dense ISM

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Figure

Figure 1. Redshifted frequencies of dense gas tracers, many of which will be ac- ac-cessible in single-tuning setups with the ngVLA at high-redshift
Figure 2. The intensity (in units of temperature) of the ground transitions of CO, C 18 O, C 17 O, HCN, HCO + , CS, and H 13 CNH 13 CO + in various clouds (labeled 1–

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