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 6.2106e-04 Jy/beam
minimum 1.1230e-04 Jy/beam
mean 1.7979e-04 Jy/beam
median 1.4355e-04 Jy/beam
sigma 8.2074e-05 Jy/beam
MAD rms 1.9157e-05 Jy/beam

RMS images

TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms

Pilot.ql.SGC3B_0.J213111_104236.10.2048.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_SGC3B_0.J213111+104236_P30582v1_2019_01_22T18_58_01.181/working/TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_0.J213111+104236_P30582v1_2019_01_22T18_58_01.181/working
Start time
2019-01-24 22:52:00.690
End
2019-01-24 22:54:32.357
Duration
0:02:31.667
Note, WebLog generation is not included in the time.

CASA logs for stage 6