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 7.5523e-04 Jy/beam
minimum 1.2763e-04 Jy/beam
mean 2.0900e-04 Jy/beam
median 1.6058e-04 Jy/beam
sigma 1.0251e-04 Jy/beam
MAD rms 1.9024e-05 Jy/beam

RMS images

TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms

Pilot.ql.SGC2D_0.J001816_084236.10.2048.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_SGC2D_0.J001816+084236_P33948v1_2019_02_12T20_19_46.464/working/TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2D_0.J001816+084236_P33948v1_2019_02_12T20_19_46.464/working
Start time
2019-02-13 23:07:29.373
End
2019-02-13 23:09:11.468
Duration
0:01:42.095
Note, WebLog generation is not included in the time.

CASA logs for stage 6