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Table 3.

Details of the images.

Clusterrelic Array Conf. Robust Taper Beam σI σQU Figs.
[μJy beam−1] [μJy beam−1] [μJy beam−1/RMSF]
8C 0212+703E C+D 0.5 18.2″ × 12.2″ 20 1, 2
C+D 0.5 20″ 29″ × 29″ 35 18 15 1, 2
8C 0212+703W C+D 0.5 18.6″ × 12.8″ 22 1, 3
C+D 0.5 20″ 33″ × 33″ 35 15 17 1, 3
Abell 3365E C+D 0.5 21.0″ × 10.6″ 28 4, 5
C+D 0.5 30″ × 30″ 28 13 16 4, 5
Abell 3365W C+D 0.5 21.0″ × 10.7″ 25 4
C+D 0.5 31″ × 31″ 28 16 19 4
PLCK G287.0+32.9 C 0.5 28.4″ × 11.7″ 33 6, 7
C 0.5 41″ × 41″ 50 11 14 6, 7
ZwCl 2341.1+0000 C+D 0.5 16.3″ × 13.5″ 17 8, 9, 10
C+D 0.5 28″ × 28″ 18 8 11 8, 9, 10

Notes. Column 1: name of the cluster with a subscript letter that specifies the relic whenever necessary; Col. 2: JVLA array configuration used to produce the image; Col. 3: robust parameter used for the Briggs weighting scheme; Col. 4: Full Width Half Maximum (FWHM) of the tapering function used to produce the image; Col. 5: FWHM of the major and minor axis of the resolution beam of the image; Col. 6: rms noise of the total intensity image; Col. 7: rms noise of the polarized intensity image produced from the Q and U images integrated over the full-band; Col. 8: average noise in the polarized intensity image computed through RM-synthesis. See Sect. 2.2 for the details on the noise calculation. Column 9: reference to the figure in this paper.

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