The properties of the reconstructed CO line emission, corrected for lensing magnification. For SDSS J0924+0219 and WFI J2033−4723, the Sérsic index, n, is fixed to a value of 1 (consistent with the value found for the dust continuum). All parameters are derived from moment maps of the reconstructed source. Note that for all except WFI J2033−4723 and PG 1115+080, the quoted sizes (but not magnifications) include an additional |$\pm 10\,\mathrm{ per\,cent}$| uncertainty due to empirical scatter in the slope of the mass profile (see Section 4.1 for details).
| . | |$\bar{\mu }_{\rm CO}$| . | RCO . | n . | ICO . | LCO . | |$L^{^{\prime }}_{\rm CO}$| . | Mdyn . |
|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (Jy km s−1) . | (L⊙) . | (K km s−1 pc2) . | (M⊙) . |
| HS 0810+2554 | 20.3 ± 0.7 | 0.27 ± 0.02 | 0.57 ± 0.06 | 0.19 ± 0.01 | (3.4 ± 0.1) × 106 | (2.6 ± 0.1) × 109 | (7 ± 1) × 109 |
| RX J0911+0551 | 13.6 ± 0.2 | 0.6 ± 0.1 | 0.56 ± 0.01 | 0.47 ± 0.01 | (4.2 ± 0.1) × 107 | (6.9 ± 0.1) × 109 | (1.1 ± 0.3) × 109 |
| SDSS J0924+0219 | 17 ± 1 | 1.7 ± 0.4 | ≡ 1.0 | 0.13 ± 0.01 | (6.4 ± 0.4) × 106 | (2.5 ± 0.2) × 108 | (6 ± 4) × 109 |
| H1413+117 | 11.1 ± 0.2 | 0.9 ± 0.1 | 0.54 ± 0.05 | 3.4 ± 0.1 | (4.8 ± 0.1) × 108 | (1.34 ± 0.02) × 1010 | (2.2 ± 0.3) × 1010 |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.23 ± 0.02 | 0.52 ± 0.03 | 0.54 ± 0.02 | (6.6 ± 0.3) × 107 | (1.4 ± 0.1) × 109 | (3.2 ± 0.3) × 109 |
| WFI J2033−4723 | 17 ± 2 | 2.1 ± 0.3 | ≡ 1.0 | 0.026 ± 0.003 | (1.5 ± 0.2) × 106 | (6.1 ± 0.7) × 107 | (3 ± 2) × 109 |
| . | |$\bar{\mu }_{\rm CO}$| . | RCO . | n . | ICO . | LCO . | |$L^{^{\prime }}_{\rm CO}$| . | Mdyn . |
|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (Jy km s−1) . | (L⊙) . | (K km s−1 pc2) . | (M⊙) . |
| HS 0810+2554 | 20.3 ± 0.7 | 0.27 ± 0.02 | 0.57 ± 0.06 | 0.19 ± 0.01 | (3.4 ± 0.1) × 106 | (2.6 ± 0.1) × 109 | (7 ± 1) × 109 |
| RX J0911+0551 | 13.6 ± 0.2 | 0.6 ± 0.1 | 0.56 ± 0.01 | 0.47 ± 0.01 | (4.2 ± 0.1) × 107 | (6.9 ± 0.1) × 109 | (1.1 ± 0.3) × 109 |
| SDSS J0924+0219 | 17 ± 1 | 1.7 ± 0.4 | ≡ 1.0 | 0.13 ± 0.01 | (6.4 ± 0.4) × 106 | (2.5 ± 0.2) × 108 | (6 ± 4) × 109 |
| H1413+117 | 11.1 ± 0.2 | 0.9 ± 0.1 | 0.54 ± 0.05 | 3.4 ± 0.1 | (4.8 ± 0.1) × 108 | (1.34 ± 0.02) × 1010 | (2.2 ± 0.3) × 1010 |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.23 ± 0.02 | 0.52 ± 0.03 | 0.54 ± 0.02 | (6.6 ± 0.3) × 107 | (1.4 ± 0.1) × 109 | (3.2 ± 0.3) × 109 |
| WFI J2033−4723 | 17 ± 2 | 2.1 ± 0.3 | ≡ 1.0 | 0.026 ± 0.003 | (1.5 ± 0.2) × 106 | (6.1 ± 0.7) × 107 | (3 ± 2) × 109 |
The properties of the reconstructed CO line emission, corrected for lensing magnification. For SDSS J0924+0219 and WFI J2033−4723, the Sérsic index, n, is fixed to a value of 1 (consistent with the value found for the dust continuum). All parameters are derived from moment maps of the reconstructed source. Note that for all except WFI J2033−4723 and PG 1115+080, the quoted sizes (but not magnifications) include an additional |$\pm 10\,\mathrm{ per\,cent}$| uncertainty due to empirical scatter in the slope of the mass profile (see Section 4.1 for details).
| . | |$\bar{\mu }_{\rm CO}$| . | RCO . | n . | ICO . | LCO . | |$L^{^{\prime }}_{\rm CO}$| . | Mdyn . |
|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (Jy km s−1) . | (L⊙) . | (K km s−1 pc2) . | (M⊙) . |
| HS 0810+2554 | 20.3 ± 0.7 | 0.27 ± 0.02 | 0.57 ± 0.06 | 0.19 ± 0.01 | (3.4 ± 0.1) × 106 | (2.6 ± 0.1) × 109 | (7 ± 1) × 109 |
| RX J0911+0551 | 13.6 ± 0.2 | 0.6 ± 0.1 | 0.56 ± 0.01 | 0.47 ± 0.01 | (4.2 ± 0.1) × 107 | (6.9 ± 0.1) × 109 | (1.1 ± 0.3) × 109 |
| SDSS J0924+0219 | 17 ± 1 | 1.7 ± 0.4 | ≡ 1.0 | 0.13 ± 0.01 | (6.4 ± 0.4) × 106 | (2.5 ± 0.2) × 108 | (6 ± 4) × 109 |
| H1413+117 | 11.1 ± 0.2 | 0.9 ± 0.1 | 0.54 ± 0.05 | 3.4 ± 0.1 | (4.8 ± 0.1) × 108 | (1.34 ± 0.02) × 1010 | (2.2 ± 0.3) × 1010 |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.23 ± 0.02 | 0.52 ± 0.03 | 0.54 ± 0.02 | (6.6 ± 0.3) × 107 | (1.4 ± 0.1) × 109 | (3.2 ± 0.3) × 109 |
| WFI J2033−4723 | 17 ± 2 | 2.1 ± 0.3 | ≡ 1.0 | 0.026 ± 0.003 | (1.5 ± 0.2) × 106 | (6.1 ± 0.7) × 107 | (3 ± 2) × 109 |
| . | |$\bar{\mu }_{\rm CO}$| . | RCO . | n . | ICO . | LCO . | |$L^{^{\prime }}_{\rm CO}$| . | Mdyn . |
|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (Jy km s−1) . | (L⊙) . | (K km s−1 pc2) . | (M⊙) . |
| HS 0810+2554 | 20.3 ± 0.7 | 0.27 ± 0.02 | 0.57 ± 0.06 | 0.19 ± 0.01 | (3.4 ± 0.1) × 106 | (2.6 ± 0.1) × 109 | (7 ± 1) × 109 |
| RX J0911+0551 | 13.6 ± 0.2 | 0.6 ± 0.1 | 0.56 ± 0.01 | 0.47 ± 0.01 | (4.2 ± 0.1) × 107 | (6.9 ± 0.1) × 109 | (1.1 ± 0.3) × 109 |
| SDSS J0924+0219 | 17 ± 1 | 1.7 ± 0.4 | ≡ 1.0 | 0.13 ± 0.01 | (6.4 ± 0.4) × 106 | (2.5 ± 0.2) × 108 | (6 ± 4) × 109 |
| H1413+117 | 11.1 ± 0.2 | 0.9 ± 0.1 | 0.54 ± 0.05 | 3.4 ± 0.1 | (4.8 ± 0.1) × 108 | (1.34 ± 0.02) × 1010 | (2.2 ± 0.3) × 1010 |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.23 ± 0.02 | 0.52 ± 0.03 | 0.54 ± 0.02 | (6.6 ± 0.3) × 107 | (1.4 ± 0.1) × 109 | (3.2 ± 0.3) × 109 |
| WFI J2033−4723 | 17 ± 2 | 2.1 ± 0.3 | ≡ 1.0 | 0.026 ± 0.003 | (1.5 ± 0.2) × 106 | (6.1 ± 0.7) × 107 | (3 ± 2) × 109 |
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