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 6.1537e-04 Jy/beam
minimum 1.1582e-04 Jy/beam
mean 1.9023e-04 Jy/beam
median 1.4949e-04 Jy/beam
sigma 8.7748e-05 Jy/beam
MAD rms 2.4935e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J013002_044235.10.2048.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_SGC1E_0.J013002+044235_P29904v1_2019_02_07T17_51_59.664/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J013002+044235_P29904v1_2019_02_07T17_51_59.664/working
Start time
2019-02-10 11:50:24.453
End
2019-02-10 11:52:49.198
Duration
0:02:24.745
Note, WebLog generation is not included in the time.

CASA logs for stage 6