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 8.9320e-04 Jy/beam
minimum 1.2427e-04 Jy/beam
mean 1.9175e-04 Jy/beam
median 1.4947e-04 Jy/beam
sigma 8.6940e-05 Jy/beam
MAD rms 1.3951e-05 Jy/beam

RMS images

TSKY0001.sb32299700.eb32302997.57550.469925937505_split.ms

Pilot.ql.Stripe82B_0_e1.J222200_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_0_e1.J222200+001724_P31247v1_2019_02_07T15_32_35.109/working/TSKY0001.sb32299700.eb32302997.57550.469925937505_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_0_e1.J222200+001724_P31247v1_2019_02_07T15_32_35.109/working
Start time
2019-02-08 21:41:34.751
End
2019-02-08 21:43:52.189
Duration
0:02:17.437
Note, WebLog generation is not included in the time.

CASA logs for stage 6