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 6.5925e-04 Jy/beam
minimum 1.2784e-04 Jy/beam
mean 2.2540e-04 Jy/beam
median 1.7511e-04 Jy/beam
sigma 9.8054e-05 Jy/beam
MAD rms 3.0726e-05 Jy/beam

RMS images

TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms

Pilot.ql.Stripe82B_1_e2.J225000_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_Stripe82B_1_e2.J225000-004235_P28021v1_2019_02_06T20_51_40.956/working/TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_1_e2.J225000-004235_P28021v1_2019_02_06T20_51_40.956/working
Start time
2019-02-07 17:47:12.535
End
2019-02-07 17:48:27.349
Duration
0:01:14.815
Note, WebLog generation is not included in the time.

CASA logs for stage 6