The properties of the reconstructed continuum emission, corrected for lensing magnification. For H1413+117, we give values after correcting the SED for photometric confusion (see Section 2.6). Note that for all except WFI J2033−4723 and PG 1115+080, the quoted sizes 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).
| . | μdust . | Rdust . | n . | |$T_{\rm d}^{\rm cold}$| . | |$T_{\rm d}^{\rm warm}$| . | β . | LFIR . | SFR . | ΣSFR . | Md . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (K) . | (K) . | . | (L⊙) . | (M⊙ yr−1) . | (M⊙ yr−1 kpc−2) . | (M⊙) . |
| HS 0810+2554 | 25 ± 4 | 0.13 ± 0.04 | 0.57 ± 0.05 | |$39^{+4}_{-5}$| | |$135^{+25}_{-18}$| | ≡ 2 | |$1.3^{+1.0}_{-0.9}\times 10^{11}$| | |$40^{+30}_{-30}$| | |$400^{+300}_{-300}$| | |$1.1^{+0.4}_{-0.5}\times 10^{7}$| |
| RX J0911+0551 | 14.8 ± 0.2 | 0.51 ± 0.03 | 0.56 ± 0.04 | |$54^{+3}_{-3}$| | – | |$1.9^{+0.1}_{-0.1}$| | |$2.3^{+0.1}_{-0.1}\times 10^{12}$| | |$750^{+50}_{-50}$| | |$500^{+100}_{-100}$| | |$5.3^{+0.9}_{-0.8}\times 10^{6}$| |
| SDSS J0924+0219 | 15.1 ± 0.7 | 1.9 ± 0.2 | 1.2 ± 0.1 | |$38^{+8}_{-7}$| | – | |$1.5^{+0.6}_{-0.4}$| | |$1.9^{+0.7}_{-0.5}\times 10^{11}$| | |$60^{+20}_{-20}$| | |$3^{+1}_{-1}$| | |$3.9^{+1.5}_{-1.4}\times 10^{7}$| |
| PG 1115+080 | 21.5 ± 0.4 | 0.14 ± 0.04 | 0.47 ± 0.01 | |$66^{+17}_{-21}$| | – | |$1.9^{+0.3}_{-0.3}$| | |$3.4^{+1.2}_{-1.0}\times 10^{11}$| | |$110^{+40}_{-30}$| | |$1000^{+400}_{-400}$| | |$2.5^{+1.5}_{-1.0}\times 10^{6}$| |
| H1413+117 | 11.2 ± 0.2 | 0.8 ± 0.1 | 0.66 ± 0.07 | |$53^{+1}_{-1}$| | |$246^{+14}_{-24}$| | |$1.88^{+0.04}_{-0.04}$| | |$4.9^{+0.2}_{-0.2}\times 10^{12}$| | |$1600^{+60}_{-60}$| | |$370^{+80}_{-80}$| | |$1.2^{+0.1}_{-0.1}\times 10^{8}$| |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.19 ± 0.02 | 0.61 ± 0.02 | |$63^{+4}_{-3}$| | – | |$1.8^{+0.1}_{-0.1}$| | |$3.1^{+1.7}_{-1.5}\times 10^{12}$| | |$1010^{+60}_{-50}$| | |$4500^{+1700}_{-1700}$| | |$3.9^{+0.1}_{0.1}\times 10^7$| |
| WFI J2033−4723 | 17.6 ± 0.9 | 2.5 ± 0.2 | 1.1 ± 0.2 | |$31^{+7}_{-5}$| | – | |$1.7^{+0.3}_{-0.3}$| | |$3.1^{+0.9}_{-0.6}\times 10^{11}$| | |$100^{+30}_{-20}$| | |$2.5^{+0.9}_{-0.7}$| | |$4.5^{+0.8}_{-0.7}\times 10^{7}$| |
| . | μdust . | Rdust . | n . | |$T_{\rm d}^{\rm cold}$| . | |$T_{\rm d}^{\rm warm}$| . | β . | LFIR . | SFR . | ΣSFR . | Md . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (K) . | (K) . | . | (L⊙) . | (M⊙ yr−1) . | (M⊙ yr−1 kpc−2) . | (M⊙) . |
| HS 0810+2554 | 25 ± 4 | 0.13 ± 0.04 | 0.57 ± 0.05 | |$39^{+4}_{-5}$| | |$135^{+25}_{-18}$| | ≡ 2 | |$1.3^{+1.0}_{-0.9}\times 10^{11}$| | |$40^{+30}_{-30}$| | |$400^{+300}_{-300}$| | |$1.1^{+0.4}_{-0.5}\times 10^{7}$| |
| RX J0911+0551 | 14.8 ± 0.2 | 0.51 ± 0.03 | 0.56 ± 0.04 | |$54^{+3}_{-3}$| | – | |$1.9^{+0.1}_{-0.1}$| | |$2.3^{+0.1}_{-0.1}\times 10^{12}$| | |$750^{+50}_{-50}$| | |$500^{+100}_{-100}$| | |$5.3^{+0.9}_{-0.8}\times 10^{6}$| |
| SDSS J0924+0219 | 15.1 ± 0.7 | 1.9 ± 0.2 | 1.2 ± 0.1 | |$38^{+8}_{-7}$| | – | |$1.5^{+0.6}_{-0.4}$| | |$1.9^{+0.7}_{-0.5}\times 10^{11}$| | |$60^{+20}_{-20}$| | |$3^{+1}_{-1}$| | |$3.9^{+1.5}_{-1.4}\times 10^{7}$| |
| PG 1115+080 | 21.5 ± 0.4 | 0.14 ± 0.04 | 0.47 ± 0.01 | |$66^{+17}_{-21}$| | – | |$1.9^{+0.3}_{-0.3}$| | |$3.4^{+1.2}_{-1.0}\times 10^{11}$| | |$110^{+40}_{-30}$| | |$1000^{+400}_{-400}$| | |$2.5^{+1.5}_{-1.0}\times 10^{6}$| |
| H1413+117 | 11.2 ± 0.2 | 0.8 ± 0.1 | 0.66 ± 0.07 | |$53^{+1}_{-1}$| | |$246^{+14}_{-24}$| | |$1.88^{+0.04}_{-0.04}$| | |$4.9^{+0.2}_{-0.2}\times 10^{12}$| | |$1600^{+60}_{-60}$| | |$370^{+80}_{-80}$| | |$1.2^{+0.1}_{-0.1}\times 10^{8}$| |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.19 ± 0.02 | 0.61 ± 0.02 | |$63^{+4}_{-3}$| | – | |$1.8^{+0.1}_{-0.1}$| | |$3.1^{+1.7}_{-1.5}\times 10^{12}$| | |$1010^{+60}_{-50}$| | |$4500^{+1700}_{-1700}$| | |$3.9^{+0.1}_{0.1}\times 10^7$| |
| WFI J2033−4723 | 17.6 ± 0.9 | 2.5 ± 0.2 | 1.1 ± 0.2 | |$31^{+7}_{-5}$| | – | |$1.7^{+0.3}_{-0.3}$| | |$3.1^{+0.9}_{-0.6}\times 10^{11}$| | |$100^{+30}_{-20}$| | |$2.5^{+0.9}_{-0.7}$| | |$4.5^{+0.8}_{-0.7}\times 10^{7}$| |
The properties of the reconstructed continuum emission, corrected for lensing magnification. For H1413+117, we give values after correcting the SED for photometric confusion (see Section 2.6). Note that for all except WFI J2033−4723 and PG 1115+080, the quoted sizes 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).
| . | μdust . | Rdust . | n . | |$T_{\rm d}^{\rm cold}$| . | |$T_{\rm d}^{\rm warm}$| . | β . | LFIR . | SFR . | ΣSFR . | Md . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (K) . | (K) . | . | (L⊙) . | (M⊙ yr−1) . | (M⊙ yr−1 kpc−2) . | (M⊙) . |
| HS 0810+2554 | 25 ± 4 | 0.13 ± 0.04 | 0.57 ± 0.05 | |$39^{+4}_{-5}$| | |$135^{+25}_{-18}$| | ≡ 2 | |$1.3^{+1.0}_{-0.9}\times 10^{11}$| | |$40^{+30}_{-30}$| | |$400^{+300}_{-300}$| | |$1.1^{+0.4}_{-0.5}\times 10^{7}$| |
| RX J0911+0551 | 14.8 ± 0.2 | 0.51 ± 0.03 | 0.56 ± 0.04 | |$54^{+3}_{-3}$| | – | |$1.9^{+0.1}_{-0.1}$| | |$2.3^{+0.1}_{-0.1}\times 10^{12}$| | |$750^{+50}_{-50}$| | |$500^{+100}_{-100}$| | |$5.3^{+0.9}_{-0.8}\times 10^{6}$| |
| SDSS J0924+0219 | 15.1 ± 0.7 | 1.9 ± 0.2 | 1.2 ± 0.1 | |$38^{+8}_{-7}$| | – | |$1.5^{+0.6}_{-0.4}$| | |$1.9^{+0.7}_{-0.5}\times 10^{11}$| | |$60^{+20}_{-20}$| | |$3^{+1}_{-1}$| | |$3.9^{+1.5}_{-1.4}\times 10^{7}$| |
| PG 1115+080 | 21.5 ± 0.4 | 0.14 ± 0.04 | 0.47 ± 0.01 | |$66^{+17}_{-21}$| | – | |$1.9^{+0.3}_{-0.3}$| | |$3.4^{+1.2}_{-1.0}\times 10^{11}$| | |$110^{+40}_{-30}$| | |$1000^{+400}_{-400}$| | |$2.5^{+1.5}_{-1.0}\times 10^{6}$| |
| H1413+117 | 11.2 ± 0.2 | 0.8 ± 0.1 | 0.66 ± 0.07 | |$53^{+1}_{-1}$| | |$246^{+14}_{-24}$| | |$1.88^{+0.04}_{-0.04}$| | |$4.9^{+0.2}_{-0.2}\times 10^{12}$| | |$1600^{+60}_{-60}$| | |$370^{+80}_{-80}$| | |$1.2^{+0.1}_{-0.1}\times 10^{8}$| |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.19 ± 0.02 | 0.61 ± 0.02 | |$63^{+4}_{-3}$| | – | |$1.8^{+0.1}_{-0.1}$| | |$3.1^{+1.7}_{-1.5}\times 10^{12}$| | |$1010^{+60}_{-50}$| | |$4500^{+1700}_{-1700}$| | |$3.9^{+0.1}_{0.1}\times 10^7$| |
| WFI J2033−4723 | 17.6 ± 0.9 | 2.5 ± 0.2 | 1.1 ± 0.2 | |$31^{+7}_{-5}$| | – | |$1.7^{+0.3}_{-0.3}$| | |$3.1^{+0.9}_{-0.6}\times 10^{11}$| | |$100^{+30}_{-20}$| | |$2.5^{+0.9}_{-0.7}$| | |$4.5^{+0.8}_{-0.7}\times 10^{7}$| |
| . | μdust . | Rdust . | n . | |$T_{\rm d}^{\rm cold}$| . | |$T_{\rm d}^{\rm warm}$| . | β . | LFIR . | SFR . | ΣSFR . | Md . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | . | (kpc) . | . | (K) . | (K) . | . | (L⊙) . | (M⊙ yr−1) . | (M⊙ yr−1 kpc−2) . | (M⊙) . |
| HS 0810+2554 | 25 ± 4 | 0.13 ± 0.04 | 0.57 ± 0.05 | |$39^{+4}_{-5}$| | |$135^{+25}_{-18}$| | ≡ 2 | |$1.3^{+1.0}_{-0.9}\times 10^{11}$| | |$40^{+30}_{-30}$| | |$400^{+300}_{-300}$| | |$1.1^{+0.4}_{-0.5}\times 10^{7}$| |
| RX J0911+0551 | 14.8 ± 0.2 | 0.51 ± 0.03 | 0.56 ± 0.04 | |$54^{+3}_{-3}$| | – | |$1.9^{+0.1}_{-0.1}$| | |$2.3^{+0.1}_{-0.1}\times 10^{12}$| | |$750^{+50}_{-50}$| | |$500^{+100}_{-100}$| | |$5.3^{+0.9}_{-0.8}\times 10^{6}$| |
| SDSS J0924+0219 | 15.1 ± 0.7 | 1.9 ± 0.2 | 1.2 ± 0.1 | |$38^{+8}_{-7}$| | – | |$1.5^{+0.6}_{-0.4}$| | |$1.9^{+0.7}_{-0.5}\times 10^{11}$| | |$60^{+20}_{-20}$| | |$3^{+1}_{-1}$| | |$3.9^{+1.5}_{-1.4}\times 10^{7}$| |
| PG 1115+080 | 21.5 ± 0.4 | 0.14 ± 0.04 | 0.47 ± 0.01 | |$66^{+17}_{-21}$| | – | |$1.9^{+0.3}_{-0.3}$| | |$3.4^{+1.2}_{-1.0}\times 10^{11}$| | |$110^{+40}_{-30}$| | |$1000^{+400}_{-400}$| | |$2.5^{+1.5}_{-1.0}\times 10^{6}$| |
| H1413+117 | 11.2 ± 0.2 | 0.8 ± 0.1 | 0.66 ± 0.07 | |$53^{+1}_{-1}$| | |$246^{+14}_{-24}$| | |$1.88^{+0.04}_{-0.04}$| | |$4.9^{+0.2}_{-0.2}\times 10^{12}$| | |$1600^{+60}_{-60}$| | |$370^{+80}_{-80}$| | |$1.2^{+0.1}_{-0.1}\times 10^{8}$| |
| WFI J2026−4536 | 19.6 ± 0.8 | 0.19 ± 0.02 | 0.61 ± 0.02 | |$63^{+4}_{-3}$| | – | |$1.8^{+0.1}_{-0.1}$| | |$3.1^{+1.7}_{-1.5}\times 10^{12}$| | |$1010^{+60}_{-50}$| | |$4500^{+1700}_{-1700}$| | |$3.9^{+0.1}_{0.1}\times 10^7$| |
| WFI J2033−4723 | 17.6 ± 0.9 | 2.5 ± 0.2 | 1.1 ± 0.2 | |$31^{+7}_{-5}$| | – | |$1.7^{+0.3}_{-0.3}$| | |$3.1^{+0.9}_{-0.6}\times 10^{11}$| | |$100^{+30}_{-20}$| | |$2.5^{+0.9}_{-0.7}$| | |$4.5^{+0.8}_{-0.7}\times 10^{7}$| |
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