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 2.0903e-03 Jy/beam
minimum 1.1299e-04 Jy/beam
mean 2.0873e-04 Jy/beam
median 1.6644e-04 Jy/beam
sigma 1.1151e-04 Jy/beam
MAD rms 5.0901e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_1.J030214_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.J030214+074236_P30391v1_2019_02_14T15_52_46.040/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_1.J030214+074236_P30391v1_2019_02_14T15_52_46.040/working
Start time
2019-02-18 09:31:37.678
End
2019-02-18 09:32:40.177
Duration
0:01:02.499
Note, WebLog generation is not included in the time.

CASA logs for stage 6