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 7.3261e-04 Jy/beam
minimum 1.1743e-04 Jy/beam
mean 1.9542e-04 Jy/beam
median 1.5563e-04 Jy/beam
sigma 9.0023e-05 Jy/beam
MAD rms 1.9869e-05 Jy/beam

RMS images

TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms

Pilot.ql.SGC2D_0.J002210_064235.10.2048.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_SGC2D_0.J002210+064235_P33929v1_2019_02_12T20_19_13.947/working/TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2D_0.J002210+064235_P33929v1_2019_02_12T20_19_13.947/working
Start time
2019-02-14 05:48:09.257
End
2019-02-14 05:50:14.158
Duration
0:02:04.901
Note, WebLog generation is not included in the time.

CASA logs for stage 6