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Table 1.

Summary of the observational properties of the VACA LoCA sample of MaDCoWS clusters.

Cluster ID Obs. date On-source time Noise rms uv range Resolution MRS
(hours) (mJy) (kλ) (arcsec) (arcmin)
MOO J0129−1640 2017-08-27 2.78 0.061 1.70 − 17.20 17.8 × 12.4 2.02
MOO J0345−2913 2017-09-03 3.15 0.055 1.91 − 17.03 18.2 × 10.6 1.80
MOO J0903+1310 2017-07-27 3.05 0.087 1.75 − 14.69 17.2 × 11.4 1.96
MOO J0917−0700 2017-05-09 2.08 0.069 2.13 − 16.51 19.4 × 9.5 1.61
MOO J1139−1706 2017-09-07 2.14 0.081 2.52 − 17.22 19.9 × 9.6 1.36
MOO J1223+2420 2017-05-08 3.07 0.061 2.09 − 13.67 16.7 × 13.2 1.64
MOO J1342−1913 2017-08-18 2.46 0.071 1.74 − 17.19 17.9 × 9.9 1.98
MOO J1414+0227 2017-09-03 3.09 0.066 1.73 − 16.30 17.0 × 9.6 1.99
MOO J2146−0320 2017-08-03 1.37 0.101 1.87 − 16.41 19.3 × 10.9 1.84
MOO J2147+1314 2017-08-19 2.61 0.062 1.54 − 14.98 18.5 × 9.6 2.23

Notes. The reported noise rms is the average noise level as measured from naturally weighted dirty images. The corresponding dirty beam is reported in the table as the nominal data resolution. The maximum recoverable scale (MRS) is instead derived from the minimum projected baseline in the full-bandwidth measurements.

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