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 8.1172e-04 Jy/beam
minimum 1.2570e-04 Jy/beam
mean 1.9581e-04 Jy/beam
median 1.5283e-04 Jy/beam
sigma 8.8615e-05 Jy/beam
MAD rms 1.9470e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J000608_124236.10.2048.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_SGC3D_0.J000608+124236_P30269v1_2019_03_06T19_41_32.547/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J000608+124236_P30269v1_2019_03_06T19_41_32.547/working
Start time
2019-03-08 16:49:35.458
End
2019-03-08 16:51:15.966
Duration
0:01:40.508
Note, WebLog generation is not included in the time.

CASA logs for stage 6