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 8.6286e-04 Jy/beam
minimum 1.2947e-04 Jy/beam
mean 2.2051e-04 Jy/beam
median 1.7113e-04 Jy/beam
sigma 1.0020e-04 Jy/beam
MAD rms 3.3860e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82B_1_e3.J225400_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_Stripe82B_1_e3.J225400+001724_P32159v1_2019_02_04T18_19_57.907/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_1_e3.J225400+001724_P32159v1_2019_02_04T18_19_57.907/working
Start time
2019-02-06 15:30:10.526
End
2019-02-06 15:31:45.091
Duration
0:01:34.565
Note, WebLog generation is not included in the time.

CASA logs for stage 6