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 3.7529e-03 Jy/beam
minimum 1.3908e-04 Jy/beam
mean 2.4832e-04 Jy/beam
median 1.7894e-04 Jy/beam
sigma 1.6498e-04 Jy/beam
MAD rms 3.1822e-05 Jy/beam

RMS images

VLASS2.1.sb38500385.eb38635359.59099.351010810184_split.ms

VLASS2.1.ql.T11t05.J031002_033000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T11t05.J031002+033000_P62233v1_2020_09_07T15_02_15.826/working/VLASS2.1.sb38500385.eb38635359.59099.351010810184_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T11t05.J031002+033000_P62233v1_2020_09_07T15_02_15.826/working
Start time
2020-10-31 11:08:11.939
End
2020-10-31 11:09:09.906
Duration
0:00:57.967
Note, WebLog generation is not included in the time.

CASA logs for stage 6