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 2.0626e-03 Jy/beam
minimum 1.1710e-04 Jy/beam
mean 2.0937e-04 Jy/beam
median 1.5627e-04 Jy/beam
sigma 1.1779e-04 Jy/beam
MAD rms 3.1931e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_1.J030603_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_1.J030603+034235_P29938v1_2019_02_14T20_03_52.047/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_1.J030603+034235_P29938v1_2019_02_14T20_03_52.047/working
Start time
2019-02-16 00:21:35.419
End
2019-02-16 00:22:47.136
Duration
0:01:11.717
Note, WebLog generation is not included in the time.

CASA logs for stage 6