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Table 1.

Summary of the new radio observations used here.

Name PID Taper Beam σRMS Diffuse sources
(″) (″ × ″) (μJy beam−1)
PSZ2G008.31–64.74 SCI-20230907-MB-02 21.9 22 × 22 12.6 RH*
SE-RR
PSZ2G056.93–55.08 SCI-20220822-MB-01 17.4 18 × 18 11.6 RH
RR*
PSZ2G172.98–53.55 SCI-20230907-MB-02 38.9 40 × 40 40.8 RH
PSZ2G225.93–19.99 SCI-20230907-MB-02 8.9 9 × 9 4.6 RH
PSZ2G239.27–26.01 SCI-20220822-MB-01 8.9 11 × 10 5.3 RH
RH
PSZ2G243.15–73.84 SCI-20230907-MB-02 9.2 10 × 10 3.7 RR-W/N
cRR-E
RH
PSZ2G262.27–35.38 SCI-20230907-MB-02 22.7 23 × 23 11.0 RR-S*
RR-N + Tailed RG
PSZ2G277.76–51.74 SCI-20230907-MB-02 25.0 25 × 25 12.6 RH
cRR
RH
PSZ2G278.58+39.16 SCI-20220822-MB-01 11.1 12 × 12 8.5 RR
Elongation
PSZ2G286.98+32.90 SCI-20220822-MB-01 9.6 10 × 10 3.9 RH
RR-NW+SE
PSZ2G313.33+61.13 SCI-20220822-MB-01 16.2 17 × 16 9.9 RH
PSZ2G346.61+35.06 SCI-20220822-MB-01 13.9 14 × 14 7.2 RH
RR

Notes. (1) Cluster name; (2) MeerKAT project ID; (3)–(5) properties of the source-subtracted, low-resolution images used to study the cluster diffuse emission, namely the Gaussian taper size applied, image resolution, and σRMS; (6) classification of the detected diffuse sources as radio halo (RH), radio relic (RR and candidate cRR), or radio galaxy (RG), while † indicates whether this source was first reported here and if it was previously indicated as a candidate.

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