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 5.5733e-04 Jy/beam
minimum 1.1020e-04 Jy/beam
mean 1.8184e-04 Jy/beam
median 1.3702e-04 Jy/beam
sigma 8.5836e-05 Jy/beam
MAD rms 1.9055e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_1.J031011_084236.10.2048.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_SGC2E_1.J031011+084236_P30403v1_2019_02_09T00_47_39.092/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_1.J031011+084236_P30403v1_2019_02_09T00_47_39.092/working
Start time
2019-02-10 17:19:33.762
End
2019-02-10 17:21:04.654
Duration
0:01:30.892
Note, WebLog generation is not included in the time.

CASA logs for stage 6