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 6.4533e-04 Jy/beam
minimum 1.0796e-04 Jy/beam
mean 1.9180e-04 Jy/beam
median 1.4510e-04 Jy/beam
sigma 9.6716e-05 Jy/beam
MAD rms 2.6298e-05 Jy/beam

RMS images

VLASS1.2.sb36663230.eb36777152.58647.27793965278_split.ms

VLASS1.2.ql.T18t28.J205829_313000.10.2048.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_T18t28.J205829+313000_P50220v1_2019_12_02T18_54_27.210/working/VLASS1.2.sb36663230.eb36777152.58647.27793965278_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t28.J205829+313000_P50220v1_2019_12_02T18_54_27.210/working
Start time
2019-12-03 18:06:45.309
End
2019-12-03 18:08:06.403
Duration
0:01:21.094
Note, WebLog generation is not included in the time.

CASA logs for stage 6