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 7.4726e-04 Jy/beam
minimum 1.1451e-04 Jy/beam
mean 1.8878e-04 Jy/beam
median 1.5053e-04 Jy/beam
sigma 9.1729e-05 Jy/beam
MAD rms 2.2505e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_0.J224435_114236.10.2048.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_0.J224435+114236_P30889v1_2019_01_22T20_35_16.893/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_0.J224435+114236_P30889v1_2019_01_22T20_35_16.893/working
Start time
2019-01-24 09:37:06.621
End
2019-01-24 09:39:40.462
Duration
0:02:33.841
Note, WebLog generation is not included in the time.

CASA logs for stage 6