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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 1.

Effect of the CMB on the Gao–Solomon relation at z = 3 for a range of kinetic temperatures with ﹩{\bar{n}}_{{{\rm{H}}}_{2}}=1\times {10}^{4}﹩ cm−3 (left) and ﹩{\bar{n}}_{{{\rm{H}}}_{2}}=1\times {10}^{5}﹩ cm−3 (right), calculated using RADEX. Data from Gao et al. (2007) and references therein: Beelen et al. (2006), Carilli et al. (2005), Solomon & Vanden Bout (2005), Wagg et al. (2005), Egami et al. (2000), Riechers et al. (2006), Isaak et al. (2004), and Greve et al. (2006).

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