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 6.6477e-04 Jy/beam
minimum 1.3496e-04 Jy/beam
mean 2.0874e-04 Jy/beam
median 1.6398e-04 Jy/beam
sigma 9.1228e-05 Jy/beam
MAD rms 1.6067e-05 Jy/beam

RMS images

TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms

Pilot.ql.Stripe82C_1_e2.J005400_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_Stripe82C_1_e2.J005400+001724_P27992v1_2019_02_04T17_36_00.300/working/TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82C_1_e2.J005400+001724_P27992v1_2019_02_04T17_36_00.300/working
Start time
2019-02-06 01:24:45.706
End
2019-02-06 01:27:08.110
Duration
0:02:22.403
Note, WebLog generation is not included in the time.

CASA logs for stage 6