Table 1.
Main properties of the galaxy clusters sample.
| SPT ID | Planck ID | RA | Dec | M500 | r500 | z | ξ |
|---|---|---|---|---|---|---|---|
| [1014 M⊙] | [arcmin] | ||||||
| SPT-CLJ0232-4421 | PSZ2 G259.98-63.43 | 38.0767° | −44.3464° | 7.45 | 4.87 | 0.28 | 23.9 |
| SPT-CLJ0438-5419 | PSZ2 G262.73-40.92 | 69.5732° | −54.3225° | 7.46 | 3.57 | 0.42 | 22.9 |
| SPT-CLJ0645-5413 | PSZ2 G263.68-22.55 | 101.3711° | −54.2272° | 7.96 | 7.89 | 0.16 | 18.3 |
| SPT-CLJ0549-6205 | PSZ2 G271.18-30.95 | 87.3287° | −62.0874° | 7.37 | 3.93 | 0.37 | 25.8 |
| SPT-CLJ0254-5857 | PSZ2 G277.76-51.74 | 43.5692° | −58.9491° | 8.65 | 3.65 | 0.44 | 14.1 |
| SPT-CLJ2344-4243 | PSZ2 G339.63-69.34 | 356.1824° | −42.7197° | 8.05 | 2.84 | 0.60 | 27.4 |
Notes. The cluster centre coordinates correspond to the X-ray peaks (see Sect. 3.2.2 for further details); the masses and the redshifts come from the Planck PSZ2 catalogue and have been used to derive r500; and ξ is the signal-to-noise ratio from the SPT catalogue (Bleem et al. 2015).
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