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 9.8923e-04 Jy/beam
minimum 1.1126e-04 Jy/beam
mean 1.8104e-04 Jy/beam
median 1.3880e-04 Jy/beam
sigma 8.8507e-05 Jy/beam
MAD rms 1.8340e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_1.J030218_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.J030218+084236_P30401v1_2019_02_09T00_47_35.584/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_1.J030218+084236_P30401v1_2019_02_09T00_47_35.584/working
Start time
2019-02-11 09:45:03.751
End
2019-02-11 09:46:38.510
Duration
0:01:34.759
Note, WebLog generation is not included in the time.

CASA logs for stage 6