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 6.2156e-04 Jy/beam
minimum 1.2108e-04 Jy/beam
mean 1.9064e-04 Jy/beam
median 1.4859e-04 Jy/beam
sigma 8.8963e-05 Jy/beam
MAD rms 1.4029e-05 Jy/beam

RMS images

TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms

Pilot.ql.Stripe82D_1_e2.J031000_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_1_e2.J031000+001724_P28381v1_2019_02_08T19_25_23.070/working/TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_1_e2.J031000+001724_P28381v1_2019_02_08T19_25_23.070/working
Start time
2019-02-10 17:42:24.438
End
2019-02-10 17:44:36.286
Duration
0:02:11.848
Note, WebLog generation is not included in the time.

CASA logs for stage 6