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Table 3.
Several examples of different probes and methods indicating similar anisotropic results to ours.
| Reference | Used method | Maximum | Significance | Angular distance from | Comments |
|---|---|---|---|---|---|
| anisotropy (l, b) | our combined results | ||||
| This work | Clusters LX–T (θ = 75°) | (303°, −27°) | 5.59σ | − | Combination of all samples |
| This work | Clusters LX–T (θ = 60°) | (281°, −16°) | 4.73σ | 23° | Our sample |
| Bengaly et al. (2017) | Infrared galaxies | (323°, −5°) | p = 0.064 | 22° | |
| Yoon et al. (2014) | Infrared galaxies | (310°, −15°) | ∼2.5σ | 13° | |
| Yang et al. (2014) | SNIa | (307°, −14°) | p = 0.046 | 13° | |
| Kalus et al. (2013) | SNIa | (325°, −19°) | 95% | 22° | z < 0.2 SNIa |
| Feindt et al. (2013) | SNIa | (298°, + 15°) | p = 0.010 | 41° | z < 0.035 SNIa, probably bulk flow |
| Mariano & Perivolaropoulos (2012) | SNIa + Quasars | (315°, −15°) | ∼99% | 16° | |
| Colin et al. (2011) | SNIa | (309°, + 19°) | p = 0.054 | 45° | z < 0.06 SNIa, probably bulk flow |
| Webb et al. (2011) | Quasars | (334°, −13°) | 4.2σ | 33° | 0.22 < z < 4.18, |
| Schwarz & Weinhorst (2007) | SNIa | (290°, −24°) | > 95% | 11° | z < 0.2 SNIa |
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