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 1.0149e-03 Jy/beam
minimum 1.3625e-04 Jy/beam
mean 2.1487e-04 Jy/beam
median 1.6812e-04 Jy/beam
sigma 9.9330e-05 Jy/beam
MAD rms 1.6445e-05 Jy/beam

RMS images

TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms

Pilot.ql.Stripe82D_0_e1.J022200_001724.10.2048.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_Stripe82D_0_e1.J022200+001724_P31613v1_2019_02_01T17_12_42.746/working/TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_0_e1.J022200+001724_P31613v1_2019_02_01T17_12_42.746/working
Start time
2019-02-03 06:08:23.533
End
2019-02-03 06:10:17.800
Duration
0:01:54.267
Note, WebLog generation is not included in the time.

CASA logs for stage 6