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 6.5314e-04 Jy/beam
minimum 1.0700e-04 Jy/beam
mean 1.7112e-04 Jy/beam
median 1.3239e-04 Jy/beam
sigma 8.1489e-05 Jy/beam
MAD rms 1.4619e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_1.J012738_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_SGC3C_1.J012738+114236_P30931v1_2019_01_22T17_26_08.308/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J012738+114236_P30931v1_2019_01_22T17_26_08.308/working
Start time
2019-01-24 09:29:59.772
End
2019-01-24 09:32:06.648
Duration
0:02:06.876
Note, WebLog generation is not included in the time.

CASA logs for stage 6