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Fig. C.1.
Gas excitation diagram for the H2 emission coming from the central part of the HATLAS090750 galaxy. The Nν, J/gν, J ratios are normalized to the value inferred from the H2(1–0)S(3) emission line transition. The population levels are well characterized by a Boltzmann distribution, suggesting that the warm H2 gas is in LTE.
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