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 6.4625e-04 Jy/beam
minimum 1.1009e-04 Jy/beam
mean 1.8614e-04 Jy/beam
median 1.3919e-04 Jy/beam
sigma 9.6104e-05 Jy/beam
MAD rms 1.9321e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_1.J023400_044235.10.2048.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_1.J023400+044235_P29940v1_2019_02_07T17_36_39.751/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_1.J023400+044235_P29940v1_2019_02_07T17_36_39.751/working
Start time
2019-02-09 20:29:02.229
End
2019-02-09 20:30:56.817
Duration
0:01:54.587
Note, WebLog generation is not included in the time.

CASA logs for stage 6