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 8.1917e-04 Jy/beam
minimum 1.2944e-04 Jy/beam
mean 2.2098e-04 Jy/beam
median 1.6411e-04 Jy/beam
sigma 1.1573e-04 Jy/beam
MAD rms 2.5561e-05 Jy/beam

RMS images

TSKY0001.sb32450678.eb32484186.57598.27566423611_split.ms

Pilot.ql.Stripe82B_2_e2.J235400_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_2_e2.J235400+001724_P27192v1_2019_02_11T18_47_07.384/working/TSKY0001.sb32450678.eb32484186.57598.27566423611_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_2_e2.J235400+001724_P27192v1_2019_02_11T18_47_07.384/working
Start time
2019-02-13 03:01:43.178
End
2019-02-13 03:03:05.127
Duration
0:01:21.949
Note, WebLog generation is not included in the time.

CASA logs for stage 6