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 6.7798e-04 Jy/beam
minimum 1.2086e-04 Jy/beam
mean 1.9922e-04 Jy/beam
median 1.5999e-04 Jy/beam
sigma 9.0177e-05 Jy/beam
MAD rms 2.6482e-05 Jy/beam

RMS images

VLASS1.2.sb36474629.eb36512955.58566.31150357639_split.ms

VLASS1.2.ql.T11t21.J133800_023000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T11t21.J133800+023000_P36451v1_2019_04_01T22_00_52.987/working/VLASS1.2.sb36474629.eb36512955.58566.31150357639_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T11t21.J133800+023000_P36451v1_2019_04_01T22_00_52.987/working
Start time
2019-04-03 03:26:58.620
End
2019-04-03 03:29:08.211
Duration
0:02:09.591
Note, WebLog generation is not included in the time.

CASA logs for stage 6