Table 10.
The cluster sample for our ℳX and ℳR comparison.
| Cluster | ℳX† | ℳR |
|---|---|---|
| A2256* | 1.8 ± 0.1 (1) | 2.7 ± 0.1 (2) |
| A2255 NE | 1.5 ± 0.2 (3) | 2.8 ± 0.4 (4) |
| A115 | 1.8 ± 0.3 (5) | 2.1 ± 0.2 (5) |
| Sausage N* | 2.7 ± 0.4 (6) | 2.7 ± 0.5 (8) |
| Sausage S* | 1.8 ± 0.5 (7) | 2.0 ± 0.2 (8) |
| A3667 NW | 2.5−0.4+0.8 (9) | 2.5 ± 0.3 (10) |
| A3667 SE | 1.8 ± 0.1 (11) | 2.5 ± 0.3 (10) |
| Coma | 2.3 ± 0.5 (12) | 1.99 ± 0.05 (13) |
| Toothbrush* | 1.8 ± 0.2 (14) | 2.8 ± 0.4 (15) |
| A3376 W | 2.8 ± 0.4 | 2.2 ± 0.4 (16) |
Notes.( * )Radio observations with LOFAR. ( † ) ℳX has been calculated as described by Sarazin et al. (2016). References: (1) Trasatti et al. (2015); (2) van Weeren et al. (2012); (3) Akamatsu et al. (2017); (4) Pizzo & de Bruyn (2009); (5) Botteon et al. (2016a); (6) Akamatsu et al. (2015); (7) Storm et al. (2018); (8) Hoang et al. (2017); (9) Sarazin et al. (2016); (10) Hindson et al. (2014); (11) Akamatsu & Kawahara (2013); (12) Akamatsu et al. (2013); (13) Thierbach et al. (2003); (14) Itahana et al. (2015); (15) van Weeren et al. (2016); (16) Kale et al. (2012).
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