Table 5.
Constraints on the peaks in the mass reconstruction signal-to-noise ratio maps including their locations (α, δ), positional uncertainties (Δα, Δδ) as estimated by bootstrapping the galaxy catalogue (we note that this underestimates the true uncertainty as found by Sommer et al. 2022), and their peak signal-to-noise ratios (S/N)peak.
| Cluster | α | δ | Δα | Δδ | Δα | Δδ | (S/N)peak |
|---|---|---|---|---|---|---|---|
| [deg J2000] | [deg J2000] | [arcsec] | [arcsec] | [kpc] | [kpc] | ||
| SPT-CL J0156−5541 | 29.04676 | −55.69426 | 9.1 | 4.8 | 76 | 41 | 2.0 |
| SPT-CL J0459−4947 | 74.92771 | −49.77739 | 8.1 | 9.6 | 69 | 81 | 2.2 |
| SPT-CL J0640−5113 | 100.08319 | −51.21488 | 6.4 | 5.5 | 53 | 46 | 2.6 |
| SPT-CL J0646-6236 | 101.63130 | −62.62127 | 1.5 | 2.2 | 12 | 18 | 5.5 |
| SPT-CL J2040−4451 | 310.24056 | −44.86349 | 4.6 | 3.7 | 39 | 31 | 3.4 |
| SPT-CL J2341−5724 | 355.34768 | −57.41418 | 7.7 | 8.1 | 64 | 68 | 2.2 |
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