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 6.3026e-04 Jy/beam
minimum 1.2282e-04 Jy/beam
mean 1.9668e-04 Jy/beam
median 1.5349e-04 Jy/beam
sigma 8.8964e-05 Jy/beam
MAD rms 2.3319e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J000201_104236.10.2048.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_SGC3D_0.J000201+104236_P30247v1_2019_03_06T19_40_57.082/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J000201+104236_P30247v1_2019_03_06T19_40_57.082/working
Start time
2019-03-08 05:52:22.651
End
2019-03-08 05:54:31.933
Duration
0:02:09.282
Note, WebLog generation is not included in the time.

CASA logs for stage 6