Extended Data Table 1 Expected number counts of CO sources

From: Compact [C ii] emitters around a C iv absorption complex at redshift 5.7

  1. The frequency is given in the rest frame. The redshift and luminosity are calculated under the assumption that the fainter line (A) detected in the ALMA data is each of the CO transitions. The expected number counts of unrelated CO sources at a line flux brighter than or equal to the observed flux are provided in the fourth column.
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