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 9.1689e-04 Jy/beam
minimum 1.2040e-04 Jy/beam
mean 2.1806e-04 Jy/beam
median 1.8281e-04 Jy/beam
sigma 9.8792e-05 Jy/beam
MAD rms 2.3241e-05 Jy/beam

RMS images

TSKY0001.sb32554861.eb32626144.57628.33101865741_split.ms

Pilot.ql.Stripe82D_2_e3.J035400_001724.10.2048.v2.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_2_e3.J035400+001724_P32762v2_2019_04_05T14_59_35.008/working/TSKY0001.sb32554861.eb32626144.57628.33101865741_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_2_e3.J035400+001724_P32762v2_2019_04_05T14_59_35.008/working
Start time
2019-04-06 23:59:00.321
End
2019-04-07 00:00:44.014
Duration
0:01:43.693
Note, WebLog generation is not included in the time.

CASA logs for stage 6