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 5.6786e-04 Jy/beam
minimum 1.1389e-04 Jy/beam
mean 1.8403e-04 Jy/beam
median 1.4616e-04 Jy/beam
sigma 8.1382e-05 Jy/beam
MAD rms 2.5518e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J014600_014235.10.2048.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.J014600+014235_P29878v1_2019_02_07T16_52_40.313/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J014600+014235_P29878v1_2019_02_07T16_52_40.313/working
Start time
2019-02-08 23:10:35.948
End
2019-02-08 23:12:23.793
Duration
0:01:47.845
Note, WebLog generation is not included in the time.

CASA logs for stage 6