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 6.3133e-04 Jy/beam
minimum 1.2856e-04 Jy/beam
mean 2.0332e-04 Jy/beam
median 1.5856e-04 Jy/beam
sigma 8.9713e-05 Jy/beam
MAD rms 2.2523e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J000202_114236.10.2048.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.J000202+114236_P30258v1_2019_03_06T19_41_14.961/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J000202+114236_P30258v1_2019_03_06T19_41_14.961/working
Start time
2019-03-08 03:37:58.705
End
2019-03-08 03:40:10.667
Duration
0:02:11.962
Note, WebLog generation is not included in the time.

CASA logs for stage 6