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 8.5338e-04 Jy/beam
minimum 1.0850e-04 Jy/beam
mean 1.7626e-04 Jy/beam
median 1.3687e-04 Jy/beam
sigma 8.5665e-05 Jy/beam
MAD rms 1.3935e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_1.J014352_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_SGC3C_1.J014352+104236_P30924v1_2019_01_22T17_25_46.910/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J014352+104236_P30924v1_2019_01_22T17_25_46.910/working
Start time
2019-01-24 08:13:54.423
End
2019-01-24 08:15:58.078
Duration
0:02:03.654
Note, WebLog generation is not included in the time.

CASA logs for stage 6