Fig. 8.

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Models of H2O population level diagrams (upper and lower panel, respectively, for ortho- and para-H2O) for our three quasar host galaxies. Each of the model shows the level volume density (weighted with their quantum degeneracy) at the NH2O, τ100, and Tdust values corresponding to the MOLPOP-CEP best-fit H2O SLED models (see Sect. 7.2). The straight lines are the analytical population diagrams computed assuming Boltzmann distribution color-coded by the excitation temperature. The green line corresponds to the LTE case (Tkin = Tex).
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