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 8.6596e-04 Jy/beam
minimum 1.3114e-04 Jy/beam
mean 2.1011e-04 Jy/beam
median 1.6561e-04 Jy/beam
sigma 9.3724e-05 Jy/beam
MAD rms 2.6191e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J003836_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.J003836+104236_P30256v1_2019_03_06T19_41_11.760/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J003836+104236_P30256v1_2019_03_06T19_41_11.760/working
Start time
2019-03-08 22:43:46.134
End
2019-03-08 22:45:24.796
Duration
0:01:38.662
Note, WebLog generation is not included in the time.

CASA logs for stage 6