Table 1.
Target list.
| Source | RA & Dec | zs | zL |  |
 |
FWHM CO(1–0) | μFIR |
|---|---|---|---|---|---|---|---|
| [J2000] | [L⊙] | [K km s−1 pc2] | [km s−1] | ||||
| SDP.81 | 09:03:11.6+00:39:07 | 3.042 | 0.23 | (43 ± 0.5) × 1012 | (54 ± 9) × 1010 | 435 ± 54 | 18.2 ± 1.2 |
| SDP.130 | 09:13:05.4−00:53:41 | 2.625 | 0.22 | (32 ± 3) × 1012 | (22 ± 6) × 1010 | 377 ± 62 | 8.6 ± 0.4 |
| HXMM.02 | 02:18:30.7−05:31:32 | 3.391 | 1.35 | (36 ± 3) × 1012 | (21 ± 2) × 1010 | 540 ± 40 | 5.3 ± 0.2 |
| J0209 | 02:09:41.3+00:15:59 | 2.553 | 0.20 | (133 ± 40) × 1012 | (54 ± 19) × 1010 | 409 ± 16 | 14.7 ± 0.3 |
| J1202 | 12:02:07.6+53:34:39 | 2.442 | 0.21 | (81 ± 40) × 1012 | (142 ± 50) × 1010 | 602 ± 21 | 25 (†) |
| J1609 | 16:09:17.8+60:45:20 | 3.256 | 0.45 | (156 ± 70) × 1012 | (334 ± 117) × 1010 | 705 ± 31 | 15.4 ± 1.0 |
Notes. Individual columns list the source position, source and lens redshift (zL, zL), sky-plane (lensed) FIR and CO(1–0) luminosities, CO(1–0) FWHM and FIR continuum magnification. LFIR inferred from modified black-body fits integrated over 8–1000 μm. (†)Derived using a Tully-Fisher argument rather than lens modelling (Harrington et al. 2021).
References. Redshifts adopted from Vlahakis (2015, SDP.81), Bussmann et al. (2013, SDP.130, HXMM.02), Geach et al. (2015, 2016, J0209), Harrington et al. (2016) and Cañameras et al. (2018, J1202 and J1609). LFIR (8–1100 μm) adopted from Rybak et al. (2020, SDP.81), Bussmann et al. (2013, SDP.130), Wardlow et al. (2013, HXMM.02), and Harrington et al. (2021). CO(1–0) line luminosities and FWHM: Valtchanov et al. (2011, SDP.81), Frayer et al. (2011, SDP.130), Riechers (in prep.) (HXMM.02, CO(1–0)), Iono et al. (2012, HXMM.02. CO(3–2)), Planck sources – Harrington et al. (2016, 2018, 2021). Lensing magnifications: Rybak et al. (2020, SDP.81), Falgarone et al. (2017, SDP.130), Bussmann et al. (2015, HXMM.02), Geach et al. (2018, J0209), Cañameras et al. (2018, J1609).
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