Table 1.
Sample of this study.
| Source | RA | Dec | zref | Transition | μ(a) | L[CII] | LIR | LFIR/MH2 | Ref. |
|---|---|---|---|---|---|---|---|---|---|
| J2000.0 | J2000.0 | [109 L⊙] | [1013 L⊙] | (L⊙/M⊙) | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| GN20 | 12:37:11.90 | 62:22:12.1 | 4.0554 | CO(2-1) | 1 | ... | 1.52 ± 0.11 | 82 ± 8 | 4(b),11 |
| ID141 | 14:24:13.93 | 02:23:04.8 | 4.243 | CO(5-4),(4-3) | 5.8 | 10.6 ± 1.7 | 1.58 ± 0.12 | 230 ± 10 | 5(b),10 |
| HDF850.1 | 12:36:52.02 | 62:12:26.0 | 5.1853 | [CII] 158 μm | 2.5 | 1.1 | 0.20 ± 0.05 | 255 ± 40 | 7(b), 17 |
| PSSJ2322+1944 | 23:22:07.18 | 19:44:22.4 | 4.1199 | CO(5-4),(4-3) | 5.3 | < 1.7 | 0.55 ± 0.10 | 132 ± 12 | 1(b),2,3,8 |
| J2054-0005 | 20:54:06.51 | −00:05:14.6 | 6.0389 | [CII] 158 μm | 1 | 3.36 ± 0.12 | 0.90 ± 0.06 | 296 ± 171 | 13,14(b),16 |
| J2310+1855 | 23:10:39.00 | 18:55:19.9 | 6.0031 | [CII] 158 μm | 1 | 8.31 ± 0.41 | 2.29 ± 0.04 | 240 ± 60 | 6(b),9,12,15 |
Notes. (1) Source name. (2) Right ascension (J2000.0). (3) Declination (J2000.0). (4) Redshift. (5) Atomic/Molecular transition used to derive redshift estimates. (6) Gravitational magnification factor. (7) [CII] 158 μm luminosity. (8) Infrared luminosity (8–1000 μm). (9) Far infrared-to-molecular gas mass ratio (computed from literature). (10) References for magnification factor, [CII] 158 μm luminosity, and molecular gas mass. The IR luminosities were estimated by fitting the dust spectral energy distribution (SED) with a modified blackbody (see Appendix B). Luminosities are corrected for gravitational magnification. References: 1: Cox et al. (2002), 2: Pety et al. (2004), 3: Solomon & Vanden Bout (2005), 4: Carilli et al. (2011), 5: Cox et al. (2011), 6: Wang et al. (2013), 7: Neri et al. (2014), 8: Valentino et al. (2018), 9: Shao et al. (2019), 10: Cheng et al. (2020), 11: Cortzen et al. (2020), 12: Li et al. (2020), 13: Pensabene et al. (2020), 14: Venemans et al. (2020) 15: Tripodi et al. (2022), 16: Salak et al. (2024), 17: Sun et al. (2024).
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