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 5.8317e-04 Jy/beam
minimum 1.1233e-04 Jy/beam
mean 1.8795e-04 Jy/beam
median 1.5312e-04 Jy/beam
sigma 7.7651e-05 Jy/beam
MAD rms 2.0956e-05 Jy/beam

RMS images

TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms

Pilot.ql.Stripe82B_1_e2.J230200_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_e2.J230200+001724_P28034v1_2019_02_04T17_38_38.272/working/TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_1_e2.J230200+001724_P28034v1_2019_02_04T17_38_38.272/working
Start time
2019-02-06 03:32:22.212
End
2019-02-06 03:34:51.717
Duration
0:02:29.505
Note, WebLog generation is not included in the time.

CASA logs for stage 6