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Table 3

H2O isotopologue observations using PACS.

Molecule Transition λ Eup θ IK Tau R Dor W Hya R Cas
[μm] [K] [′′] [× 10-16 W m-2] [× 10-16 W m-2] [× 10-16 W m-2] [× 10-16 W m-2]

o-H217O 22,1 → 21,2 180.33 114 13 blend x 0.71 (30%) 0.17 (46%)
62,5 → 61,6 94.91 794 9 3.49 (25%) blend blend blend
o-H218O 22,1 → 21,2 183.53 192 13 0.91 (29%) x x x
22,1 → 11,0 109.35 192 10 4.30 (26%) 2.15 (53%) x 0.69 (45%)
61,6 → 50,5 82.44 641 9 blend blend 2.25 (25%) blend
33,0 → 22,1 67.19 406 9 2.66 (40%) x x x
62,5 → 51,4 65.75 792 9 1.23 (61%) x x x
43,2 → 32,1 59.35 546 9 2.88 (26%) x x x
p-H218O 31,3 → 20,2 139.59 204 11 0.99 (38%) x x x
32,2 → 21,1 90.94 295 9 1.51 (26%) x 1.54 (50%) x

Notes. Eup is the energy of the upper level in the transition, θ is the half power beam width of the telescope at the corresponding frequency. The integrated line strengths are given for each source and transition. (x) indicates a non-detection and numbers in brackets indicate percentage errors.

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