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Table 2.
Galaxy clusters with known dynamical states from literature used to calibrate our method.
| Cluster | Dynamical state | Reference |
|---|---|---|
| Abell 141 | Disturbed | Cassano et al. (2010) |
| Abell 267 | Relaxed | Cassano et al. (2010) |
| Abell 384 | Relaxed | Cuciti et al. (2021) |
| Abell 402 | Relaxed | Cuciti et al. (2021) |
| Abell 2537 | Relaxed | Cassano et al. (2010) |
| Abell 2631 | Disturbed | Cuciti et al. (2021) |
| Abell 2697 | Relaxed | Cuciti et al. (2021) |
| Abell 2744 | Disturbed | Cassano et al. (2010) |
| Abell 2813 | Relaxed | Kesebonye et al. (2023) |
| Abell 2895 | Disturbed | Kesebonye et al. (2023) |
| Abell 3017 | Intermediate | Lovisari et al. (2017) |
| Abell 3041 | Disturbed | Cuciti et al. (2021) |
| Abell 3088 | Relaxed | Cassano et al. (2010) |
| Abell 3322 | Intermediate | Lovisari et al. (2017) |
| Abell 3343 | Relaxed | Kesebonye et al. (2023) |
| Abell 3364 | Relaxed | Lovisari et al. (2017) |
| Abell 3378 | Relaxed | Lovisari et al. (2017) |
| Abell 3739 | Relaxed | Lovisari et al. (2017) |
| Abell 3827 | Relaxed | Lovisari et al. (2017) |
| Abell S295 | Disturbed | Kesebonye et al. (2023) |
| Abell S520 | Disturbed | Kesebonye et al. (2023) |
| Abell S1063 | Relaxed | Kesebonye et al. (2023) |
| ACT-CLJ0217-5245 | Disturbed | Kesebonye et al. (2023) |
| RXC J0528.2-2942 | Relaxed | Kesebonye et al. (2023) |
| RXC J2023.4-5535 | Disturbed | Kesebonye et al. (2023) |
| SPT-CLJ0232-4421 | Relaxed | Kesebonye et al. (2023) |
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