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Table 3
SMGs and QSOs from the literature with published [CI]2–1, CO(7–6) and H2O detections along with published IR luminosities used for comparison to the Spiderweb galaxy.
| Source | z | μ | SdVCO(7–6) | SdV[ CI ] | Reference |
| [Jy km s-1] | [Jy km s-1] | ||||
|
|
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| SDP.11 | 1.7860 | 18 | 18 ± 14 | 31 ± 14 | Lupu et al. (2012), Ferkinhoff et al. (2014) |
| SDP17.b | 2.3080 | 4.3 | 11 ± 7 | 13 ± 7 | Lupu et al. (2012) |
| SMMJ2135-0102 | 2.3259 | 32.5 | 12.6 ± 0.6 | 16.2 ± 0.6 | Danielson et al. (2011) |
| SMMJ16359+6612 | 2.5160 | 22 | 3.3 ± 1.4 | 1.6 ± 0.3 | Kneib et al. (2005), Walter et al. (2011) |
| H1413+117 | 2.5585 | 11 | 44.6 ± 3.1 | 5.2 ± 0.3 | Alloin et al. (1997), Weiß et al. (2003) |
| SMMJ14011+0252 | 2.5650 | 23 | 3.2 ± 0.5 | 3.1 ± 0.3 | Downes & Solomon (2003), Walter et al. (2011) |
| SDP.81 | 3.0370 | 9.5 | 12 ± 4 | < 6.5 | Lupu et al. (2012) |
| MM18423+5938 | 3.9296 | 12 | 3.9 ± 0.5 | 4.2 ± 0.8 | Lestrade et al. (2010) |
| ID141 | 4.2430 | 10–30 | 6.5 ± 1.4 | 3.4 ± 1.1 | Cox et al. (2011) |
| HFLS3 | 6.3369 | 2.2 | 2.2 ± 0.3 | 0.5 ± 0.4 | Riechers et al. (2013) |
|
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| SdVH2O | μ L IR | Reference | |||
| [Jy km s-1] | [1013L⊙] | ||||
|
|
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| SDP9 | 1.574 | 8.5 | 14.4 ± 1.1 | 4.4 | Lupu et al. (2012) |
| NAv1144 | 2.202 | 5.3 | 7.5 ± 0.9 | 5.7 | Omont et al. (2013) |
| G15v2779 | 4.244 | 4.1 | 4.1 ± 0.6 | 8.5 | Omont et al. (2013) |
| APM08279+5255 | 3.912 | 4.0 | <1.1 | 20 | van der Werf et al. (2011), Walter et al. (2011) |
| HFLS3 | 6.3369 | 2.2 | 2.6 ± 0.8 | 4.2 | Riechers et al. (2013) |
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