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 8.6129e-04 Jy/beam
minimum 1.3309e-04 Jy/beam
mean 2.1715e-04 Jy/beam
median 1.6786e-04 Jy/beam
sigma 1.1330e-04 Jy/beam
MAD rms 2.4654e-05 Jy/beam

RMS images

TSKY0001.sb32297857.eb32303010.57551.487867233795_split.ms

Pilot.ql.Stripe82C_0_e1.J003800_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_0_e1.J003800+001724_P31414v1_2019_02_01T17_03_41.532/working/TSKY0001.sb32297857.eb32303010.57551.487867233795_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82C_0_e1.J003800+001724_P31414v1_2019_02_01T17_03_41.532/working
Start time
2019-02-03 05:50:04.955
End
2019-02-03 05:52:18.221
Duration
0:02:13.267
Note, WebLog generation is not included in the time.

CASA logs for stage 6