Table B.1
Beam-matched H2O+, H2O line and infrared luminosities from local detections (Herschel SPIRE/FTS archive) and high-redshift Herschel lensed galaxies.
| Source | 202–111 (5/2−3/2) | 211–202 (5/2−5/2) | L IR−beam | L H2O |
| 106 L⊙ | 106 L⊙ | 1011 L⊙ | 106 L⊙ | |
|
|
||||
| Local ULIRGs | ||||
| ESO320-G030 | 0.4 ± 0.1 | – | 1.5 | 0.9 |
| CGCG049-057 | 0.3 ± 0.1 | 0.7 ± 0.2 | 1.9 | 1.6 |
| NGC 2623 | 0.5 ± 0.2 | 0.7 ± 0.3 | 3.5 | 2.0 |
| Arp299-A | 0.8 ± 0.2 | 0.7 ± 0.3 | 5.4 | 1.3 |
| Arp220 | 3.7 ± 0.8 | 3.5 ± 0.9 | 16.2 | 15.2 |
| IRAS13120-5453 | 3.6 ± 1.2 | 2.4 ± 1.0 | 28.2 | 10.7 |
| IRASF17207-0014 | 6.8 ± 2.2 | 6.3 ± 2.2 | 24.6 | 15.5 |
| Mrk231 | 2.6 ± 1.0 | 3.0 ± 1.5 | 32.4 | 9.3 |
|
|
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| High-redshift lensed galaxies | ||||
| NCv1.143 | 28.7 ± 7.2 | 28.6 ± 7.2 | 113.6 | 89.7 |
| G09v1.97 | 35.8 ± 9.0 | – | 211.4 | 106.6 |
| G15v2.779 | – | 55.8 ± 15.9 | 270.0 | 266.0 |
| HFLS3 | – | 261.8 ± 200.3 | 364.0 | 737.8 |
Notes. Luminosity of H2O+ fine structure lines 202–111 (5/2−3/2) (742.1 GHz), 211–202 (5/2−5/2) (746.5 GHz), and H2O(211–202). As for the local sources the Herschel SPIRE/FTS beam is smaller than the entire source for some galaxies, here LIR−beam represents the LIR from the same beam area as the measured emission line (a full description will be given by Liu et al., in prep.). LH2O is the luminosity of H2O(211–202). HFLS3 data are taken from Riechers et al. (2013).
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