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 6.9503e-04 Jy/beam
minimum 1.3413e-04 Jy/beam
mean 2.1206e-04 Jy/beam
median 1.6723e-04 Jy/beam
sigma 9.7289e-05 Jy/beam
MAD rms 1.7402e-05 Jy/beam

RMS images

TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms

Pilot.ql.Stripe82D_1_e1.J031400_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_e1.J031400+001724_P31596v1_2019_02_01T17_11_56.083/working/TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_1_e1.J031400+001724_P31596v1_2019_02_01T17_11_56.083/working
Start time
2019-02-03 07:38:32.637
End
2019-02-03 07:40:36.734
Duration
0:02:04.098
Note, WebLog generation is not included in the time.

CASA logs for stage 6