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 8.2685e-04 Jy/beam
minimum 1.3523e-04 Jy/beam
mean 2.2265e-04 Jy/beam
median 1.8027e-04 Jy/beam
sigma 1.0006e-04 Jy/beam
MAD rms 3.4210e-05 Jy/beam

RMS images

TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms

Pilot.ql.Stripe82D_1_e1.J031800_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.J031800+001724_P31597v1_2019_02_01T17_11_59.790/working/TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_1_e1.J031800+001724_P31597v1_2019_02_01T17_11_59.790/working
Start time
2019-02-02 19:28:08.154
End
2019-02-02 19:29:58.772
Duration
0:01:50.618
Note, WebLog generation is not included in the time.

CASA logs for stage 6