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Table 7
Overview of CO detections that are not directly associated with the radio galaxy.
| HzRG | z | CO detection | Separationa | CO/dust association | Reference | |
|
|
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| MRC0114-211 | 1.402 | CO(1−0) | 35 kpc | no | Emonts et al. (2014); Nilsson et al. (in prep.) | |
| MRC0152-209 | 1.921 | CO(1−0)/CO(6−5) | 10 kpc | yes | Emonts et al. (2014, 2015) | |
| MRC0156-252 | 2.016 | CO(1−0) | 60 kpc | no | Emonts et al. (2014); Nilsson et al. (in prep.) | |
| MRC2048-272 | 2.060 | CO(1−0) | 55 kpc | no | Emonts et al. (2014); Nilsson et al. (in prep.) | |
| MRC1138-262 | 2.161 | CO(1−0) | 30−40 kpc | yes | Emonts et al. (2013); Gullberg et al. (in prep.) | |
| TXS0828+193 | 2.572 | CO(3−2) | 80 kpc | no | Nesvadba et al. (2009) | |
| MRC0943-242 | 2.923 | CO(8−7) | 80 kpc | no | This work | |
| B3J2330+3927 | 3.086 | CO(1−0)/CO(4−3) | 30 kpc | yes | Ivison et al. (2012) | |
| 4C41.17 | 3.798 | CO(4−3) | 13 kpc | yes | De Breuck et al. (2005) | |
| 4C60.07 | 3.8 | CO(1−0)/CO(4−3) | 30 kpc | yes | Ivison et al. (2008), Greve et al. (2004) | |
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