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 7.8193e-04 Jy/beam
minimum 1.2262e-04 Jy/beam
mean 1.9813e-04 Jy/beam
median 1.5545e-04 Jy/beam
sigma 8.7732e-05 Jy/beam
MAD rms 1.8188e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82A_1_e3.J205800_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_Stripe82A_1_e3.J205800+001724_P32140v1_2019_01_31T18_17_40.815/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_1_e3.J205800+001724_P32140v1_2019_01_31T18_17_40.815/working
Start time
2019-02-02 06:44:24.813
End
2019-02-02 06:46:32.476
Duration
0:02:07.663
Note, WebLog generation is not included in the time.

CASA logs for stage 6