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 6.2937e-04 Jy/beam
minimum 1.2658e-04 Jy/beam
mean 2.0809e-04 Jy/beam
median 1.6113e-04 Jy/beam
sigma 9.1176e-05 Jy/beam
MAD rms 2.5373e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82A_1_e3.J210600_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_Stripe82A_1_e3.J210600+001724_P32142v1_2019_02_01T17_03_52.352/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_1_e3.J210600+001724_P32142v1_2019_02_01T17_03_52.352/working
Start time
2019-02-03 03:41:56.504
End
2019-02-03 03:43:16.988
Duration
0:01:20.484
Note, WebLog generation is not included in the time.

CASA logs for stage 6