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The Role of the CMB in Redshift Related Departures from the Gao–Solomon Relation

  • Authors: R. Tunnard, and T. R. Greve

2017 The Astrophysical Journal 849 37.

  • Provider: AAS Journals

Caption: Figure 5.

Galaxy integrated line luminosities, relative to those at z = 0, as functions of redshift for the toy models. Left: HCN(1−0). Right: CO(1−0). The loss of contrast against the CMB is evident even for the NGC 1068 analogue. In both subplots the constant density model (CD) is also plotted in gray with crosses.

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