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 6.4244e-04 Jy/beam
minimum 1.1280e-04 Jy/beam
mean 1.8218e-04 Jy/beam
median 1.4463e-04 Jy/beam
sigma 8.0901e-05 Jy/beam
MAD rms 2.5110e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J013000_024235.10.2048.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.J013000+024235_P29884v1_2019_02_07T17_02_50.014/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J013000+024235_P29884v1_2019_02_07T17_02_50.014/working
Start time
2019-02-09 10:02:53.104
End
2019-02-09 10:05:23.025
Duration
0:02:29.921
Note, WebLog generation is not included in the time.

CASA logs for stage 6