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 6.6461e-04 Jy/beam
minimum 1.2193e-04 Jy/beam
mean 1.9362e-04 Jy/beam
median 1.4943e-04 Jy/beam
sigma 8.9046e-05 Jy/beam
MAD rms 1.5384e-05 Jy/beam

RMS images

TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms

Pilot.ql.Stripe82D_1_e2.J025000_004235.10.2048.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.J025000-004235_P28366v1_2019_02_08T19_24_57.973/working/TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_1_e2.J025000-004235_P28366v1_2019_02_08T19_24_57.973/working
Start time
2019-02-10 03:36:49.479
End
2019-02-10 03:38:46.342
Duration
0:01:56.863
Note, WebLog generation is not included in the time.

CASA logs for stage 6