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 9.4542e-04 Jy/beam
minimum 1.2401e-04 Jy/beam
mean 2.0369e-04 Jy/beam
median 1.5700e-04 Jy/beam
sigma 9.4336e-05 Jy/beam
MAD rms 2.5267e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J000202_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.J000202+124236_P30268v1_2019_03_06T19_41_30.951/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J000202+124236_P30268v1_2019_03_06T19_41_30.951/working
Start time
2019-03-08 07:32:32.238
End
2019-03-08 07:34:18.649
Duration
0:01:46.411
Note, WebLog generation is not included in the time.

CASA logs for stage 6