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 6.1441e-04 Jy/beam
minimum 1.1533e-04 Jy/beam
mean 1.8669e-04 Jy/beam
median 1.4031e-04 Jy/beam
sigma 9.1089e-05 Jy/beam
MAD rms 1.7211e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J011400_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_0.J011400+044235_P29900v1_2019_02_07T17_51_47.222/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J011400+044235_P29900v1_2019_02_07T17_51_47.222/working
Start time
2019-02-09 00:02:19.339
End
2019-02-09 00:04:21.791
Duration
0:02:02.452
Note, WebLog generation is not included in the time.

CASA logs for stage 6