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 5.8386e-04 Jy/beam
minimum 1.2429e-04 Jy/beam
mean 1.9183e-04 Jy/beam
median 1.5119e-04 Jy/beam
sigma 8.2799e-05 Jy/beam
MAD rms 1.7837e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J002620_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_SGC3D_0.J002620+094236_P30242v1_2019_03_06T19_40_49.126/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J002620+094236_P30242v1_2019_03_06T19_40_49.126/working
Start time
2019-03-08 13:06:03.949
End
2019-03-08 13:08:12.720
Duration
0:02:08.771
Note, WebLog generation is not included in the time.

CASA logs for stage 6