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 6.0027e-04 Jy/beam
minimum 1.2197e-04 Jy/beam
mean 1.8723e-04 Jy/beam
median 1.4638e-04 Jy/beam
sigma 8.3317e-05 Jy/beam
MAD rms 1.4218e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J002630_114236.10.2048.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.J002630+114236_P30264v1_2019_03_06T19_41_24.553/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J002630+114236_P30264v1_2019_03_06T19_41_24.553/working
Start time
2019-03-08 14:44:10.862
End
2019-03-08 14:46:41.382
Duration
0:02:30.520
Note, WebLog generation is not included in the time.

CASA logs for stage 6