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Submillimeter H2O and H2O+ emission in lensed ultra and hyper luminous infrared galaxies at z ~ 2–4

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Figure

Fig. 1. Energy level diagrams of H1the photon labeled. The light blue dashed arrow is the transition frompara-Hrespectively
Table 2. Previously observed properties of the sample.
Fig. 2a. Spatially integrated spectra of HNAv1.195, all the2O in the six sources with both J = 2 para-H2O and J = 3 ortho-H2O lines observed
Table 3. Observed CO line properties using the IRAM 30 m/EMIR.
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