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 1.2140e-03 Jy/beam
minimum 1.2552e-04 Jy/beam
mean 2.0517e-04 Jy/beam
median 1.5948e-04 Jy/beam
sigma 9.4710e-05 Jy/beam
MAD rms 2.6235e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_0.J003829_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.J003829+094236_P30245v1_2019_03_06T19_40_53.903/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_0.J003829+094236_P30245v1_2019_03_06T19_40_53.903/working
Start time
2019-03-08 16:47:56.878
End
2019-03-08 16:49:25.194
Duration
0:01:28.317
Note, WebLog generation is not included in the time.

CASA logs for stage 6