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 5.8366e-04 Jy/beam
minimum 1.1409e-04 Jy/beam
mean 1.7742e-04 Jy/beam
median 1.3621e-04 Jy/beam
sigma 8.1684e-05 Jy/beam
MAD rms 1.3743e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_0.J012603_054235.10.2048.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_0.J012603+054235_P30407v1_2019_02_09T00_47_45.687/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_0.J012603+054235_P30407v1_2019_02_09T00_47_45.687/working
Start time
2019-02-11 05:02:00.527
End
2019-02-11 05:03:47.028
Duration
0:01:46.500
Note, WebLog generation is not included in the time.

CASA logs for stage 6