Table 2.

Observed line intensities, line luminosities, and continuum flux densities for the ALMA observations, uncorrected for lensing magnification. A 5 per cent error in amplitude calibration should be assumed for the continuum flux density.

IlineLline|$L^{\prime }_{\rm line}$|ScontReference
(Jy km s−1)(L)(K km s−1 pc2)(mJy)
H2O (414–321)1.0 ± 0.1(5.3 ± 0.6) × 107(3.0 ± 0.4) × 101027This work
H2O (616–523)0.30 ± 0.03(9.5 ± 0.9) × 105(2.7 × 0.3) × 101271Castangia et al. (2011)
CO (11–10)6.4 ± 0.3(1.16 ± 0.06) × 109(1.78 ± 0.09) × 101024This work; Stacey & McKean (2018)
IlineLline|$L^{\prime }_{\rm line}$|ScontReference
(Jy km s−1)(L)(K km s−1 pc2)(mJy)
H2O (414–321)1.0 ± 0.1(5.3 ± 0.6) × 107(3.0 ± 0.4) × 101027This work
H2O (616–523)0.30 ± 0.03(9.5 ± 0.9) × 105(2.7 × 0.3) × 101271Castangia et al. (2011)
CO (11–10)6.4 ± 0.3(1.16 ± 0.06) × 109(1.78 ± 0.09) × 101024This work; Stacey & McKean (2018)
Table 2.

Observed line intensities, line luminosities, and continuum flux densities for the ALMA observations, uncorrected for lensing magnification. A 5 per cent error in amplitude calibration should be assumed for the continuum flux density.

IlineLline|$L^{\prime }_{\rm line}$|ScontReference
(Jy km s−1)(L)(K km s−1 pc2)(mJy)
H2O (414–321)1.0 ± 0.1(5.3 ± 0.6) × 107(3.0 ± 0.4) × 101027This work
H2O (616–523)0.30 ± 0.03(9.5 ± 0.9) × 105(2.7 × 0.3) × 101271Castangia et al. (2011)
CO (11–10)6.4 ± 0.3(1.16 ± 0.06) × 109(1.78 ± 0.09) × 101024This work; Stacey & McKean (2018)
IlineLline|$L^{\prime }_{\rm line}$|ScontReference
(Jy km s−1)(L)(K km s−1 pc2)(mJy)
H2O (414–321)1.0 ± 0.1(5.3 ± 0.6) × 107(3.0 ± 0.4) × 101027This work
H2O (616–523)0.30 ± 0.03(9.5 ± 0.9) × 105(2.7 × 0.3) × 101271Castangia et al. (2011)
CO (11–10)6.4 ± 0.3(1.16 ± 0.06) × 109(1.78 ± 0.09) × 101024This work; Stacey & McKean (2018)
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