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Table 1

Highest S/N noise clusters in the Planck catalogue.

Cluster S/N z Planck valid. Δ(∑ χ2)CO−y Validation Cosmology Q N

PSZ2 G075.71+13.51 48.98511 0.05570 21 893.456 CLG T 0.994
PSZ2 G110.98+31.73 40.75489 0.05810 21 294.893 CLG T 0.992
PSZ2 G272.08-40.16 39.99466 0.05890 21 492.870 CLG T 0.993
PSZ2 G239.29+24.75 36.24374 0.05420 21 192.400 CLG T 0.993
PSZ2 G057.80+88.00 35.69822 0.02310 21 418.131 CLG T 0.992
PSZ2 G006.76+30.45 35.01054 0.20300 21 137.806 CLG F 0.994
PSZ2 G324.59-11.52 32.40285 0.05080 21 321.450 CLG F 0.993
PSZ2 G044.20+48.66 28.38608 0.08940 21 127.431 CLG T 0.994
PSZ2 G266.04-21.25 28.38260 0.29650 21 103.555 CLG T 0.993
PSZ2 G072.62+41.46 27.43035 0.22800 20 88.383 CLG T 0.994

Notes. All columns except for Δ( ∑ χ2)CO−y and validation columns are from the Planck catalogue. The key to Planck validation column can be found in (Planck Collaboration XXVII 2016) and tells which external source was use for validation, a −1 in this column mean an unconfirmed candidate. The last columns tells whether this source is included in the sample used for cosmological analysis. Also shown is the quality factor from Planck catalogue, QN (Aghanim et al. 2015) with QN > 0.4 suggested by the Planck collaboration as the criterion to describe the good quality clusters. The full table is available at the CDS.

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