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 7.5323e-04 Jy/beam
minimum 1.1612e-04 Jy/beam
mean 2.0757e-04 Jy/beam
median 1.5100e-04 Jy/beam
sigma 1.1028e-04 Jy/beam
MAD rms 3.1578e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_1.J020209_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_SGC3C_1.J020209+094236_P30918v1_2019_01_22T20_46_11.128/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J020209+094236_P30918v1_2019_01_22T20_46_11.128/working
Start time
2019-01-23 09:18:32.338
End
2019-01-23 09:19:48.629
Duration
0:01:16.291
Note, WebLog generation is not included in the time.

CASA logs for stage 6