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Table 1.

Properties of the galaxy cluster sample.

Cluster name zl ξ Coordinates centres (deg J2000)
M500c, SZ
SZ α SZ δ X-ray α X-ray δ [1014M/h70]
SPT-CL J0156−5541 1.288 (a) 6.98 29.04490 −55.69801 29.0405 −55.6976
SPT-CL J0205−5829 1.322 (b) 10.40 31.44282 −58.48521 31.4459 −58.4849
SPT-CL J0313−5334 1.474 (a) 6.09 48.48090 −53.57809 48.4813 −53.5718
SPT-CL J0459−4947 1.710 (d) 6.29 74.92693 −49.78724 74.9240 −49.7823
SPT-CL J0607−4448 1.401 (a) 6.44 91.89841 −44.80333 91.8940 −44.8050
SPT-CL J0640−5113 1.316 (a) 6.86 100.06452 −51.22045 100.0720 −51.2176
SPT-CL J0646−6236 0.995 (e) 8.67 101.63906 −62.61360 (f)
SPT-CL J2040−4451 1.478 (c) 6.72 310.24832 −44.86023 310.2417 −44.8620
SPT-CL J2341−5724 1.259 (a) 6.87 355.35683 −57.41580 355.3533 −57.4166

Notes. We list cluster names, SZ significance ξ, SZ coordinates of the centre and SZ masses as presented in B19. The X-ray coordinates correspond to the centroid positions estimated by McDonald et al. (2017).

(a)

Spectroscopic redshifts by Khullar et al. (2019).

(b)

Spectroscopic redshift from Stalder et al. (2013).

(c)

Spectroscopic redshift from Bayliss et al. (2014).

(d)

Best redshift constraint currently available (based on a spectral analysis of XMM-Newton data, using the 6.7 keV Fe emission line complex, Mantz et al. 2020).

(e)

Observation design and data reduction followed the same procedures as described in Khullar et al. (2019). More general results will be discussed in a future paper on high-z spectroscopic measurements of SPT clusters.

(f)

We list the SZ mass recalculated at the updated redshift of the cluster.

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