RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 5.8705e-04 Jy/beam
minimum 1.0921e-04 Jy/beam
mean 1.7409e-04 Jy/beam
median 1.3443e-04 Jy/beam
sigma 8.1803e-05 Jy/beam
MAD rms 1.6059e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_1.J014356_114236.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J014356+114236_P30935v1_2019_01_22T17_26_25.893/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J014356+114236_P30935v1_2019_01_22T17_26_25.893/working
Start time
2019-01-24 13:24:35.666
End
2019-01-24 13:26:33.141
Duration
0:01:57.475
Note, WebLog generation is not included in the time.

CASA logs for stage 6