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 1.2474e-03 Jy/beam
minimum 1.1064e-04 Jy/beam
mean 1.8421e-04 Jy/beam
median 1.4402e-04 Jy/beam
sigma 8.8013e-05 Jy/beam
MAD rms 2.1036e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J012200_034235.10.2048.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_SGC1E_0.J012200+034235_P29892v1_2019_02_07T17_12_47.111/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J012200+034235_P29892v1_2019_02_07T17_12_47.111/working
Start time
2019-02-10 15:45:46.581
End
2019-02-10 15:48:09.560
Duration
0:02:22.979
Note, WebLog generation is not included in the time.

CASA logs for stage 6