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 7.9230e-04 Jy/beam
minimum 1.1098e-04 Jy/beam
mean 1.8210e-04 Jy/beam
median 1.4312e-04 Jy/beam
sigma 8.2646e-05 Jy/beam
MAD rms 2.2829e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_1.J030616_074236.10.2048.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.J030616+074236_P30392v1_2019_02_09T00_47_20.780/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_1.J030616+074236_P30392v1_2019_02_09T00_47_20.780/working
Start time
2019-02-11 16:02:38.988
End
2019-02-11 16:04:20.983
Duration
0:01:41.996
Note, WebLog generation is not included in the time.

CASA logs for stage 6