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 6.7979e-04 Jy/beam
minimum 1.1065e-04 Jy/beam
mean 1.9102e-04 Jy/beam
median 1.4810e-04 Jy/beam
sigma 9.1450e-05 Jy/beam
MAD rms 3.1221e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J011400_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.J011400+014235_P29870v1_2019_02_06T23_51_57.088/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J011400+014235_P29870v1_2019_02_06T23_51_57.088/working
Start time
2019-02-07 20:52:38.549
End
2019-02-07 20:54:10.608
Duration
0:01:32.059
Note, WebLog generation is not included in the time.

CASA logs for stage 6