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 6.1359e-04 Jy/beam
minimum 1.1476e-04 Jy/beam
mean 1.8974e-04 Jy/beam
median 1.4364e-04 Jy/beam
sigma 8.8550e-05 Jy/beam
MAD rms 1.9082e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J000201_094236.10.2048.v2.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+094236_P30236v2_2019_03_11T09_01_31.738/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J000201+094236_P30236v2_2019_03_11T09_01_31.738/working
Start time
2019-03-12 02:44:55.334
End
2019-03-12 02:46:31.474
Duration
0:01:36.140
Note, WebLog generation is not included in the time.

CASA logs for stage 6