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 6.3090e-04 Jy/beam
minimum 1.1724e-04 Jy/beam
mean 1.8778e-04 Jy/beam
median 1.4271e-04 Jy/beam
sigma 9.3221e-05 Jy/beam
MAD rms 1.6474e-05 Jy/beam

RMS images

TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms

Pilot.ql.SGC3B_1.J233728_094236.10.2048.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_1.J233728+094236_P30530v1_2019_01_22T18_55_59.220/working/TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_1.J233728+094236_P30530v1_2019_01_22T18_55_59.220/working
Start time
2019-01-24 07:09:57.977
End
2019-01-24 07:12:11.480
Duration
0:02:13.503
Note, WebLog generation is not included in the time.

CASA logs for stage 6