Table 1.
Possible anisotropy causes that can be traced by each cluster scaling relation.
| Measurement | LX | YSZ | R | LBCG | T |
|---|---|---|---|---|---|
| LX | 1 | 2*,3* | 1 | 1,2,3 | |
| YSZ | 2*,3* | 4 | 1*,2,3 | ||
| R | 2*,3* | 1*,2,3 | |||
| LBCG | 1*,2,3 |
Notes. 1: Unaccounted X-ray absorption effects. 2: BFs. 3: Cosmological anisotropies. 4: Expected to look isotropic if no systematics exist in the measurements or methodology. The star * means that the detection of an underlying effect is rather weak, and cannot be achieved by current samples.
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