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 6.4781e-04 Jy/beam
minimum 1.1919e-04 Jy/beam
mean 1.9100e-04 Jy/beam
median 1.4591e-04 Jy/beam
sigma 9.4094e-05 Jy/beam
MAD rms 1.5514e-05 Jy/beam

RMS images

TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms

Pilot.ql.Stripe82D_0_e2.J023000_004235.10.2048.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_0_e2.J023000-004235_P28331v1_2019_02_08T19_23_59.185/working/TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_0_e2.J023000-004235_P28331v1_2019_02_08T19_23_59.185/working
Start time
2019-02-09 23:05:07.097
End
2019-02-09 23:07:03.123
Duration
0:01:56.026
Note, WebLog generation is not included in the time.

CASA logs for stage 6