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 6.4644e-04 Jy/beam
minimum 1.1506e-04 Jy/beam
mean 2.0743e-04 Jy/beam
median 1.7314e-04 Jy/beam
sigma 9.2941e-05 Jy/beam
MAD rms 5.2729e-05 Jy/beam

RMS images

VLASS1.2.sb36458312.eb36595350.58593.54284034722_split.ms

VLASS1.2.ql.T20t30.J235832_373000.10.2048.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_T20t30.J235832+373000_P44904v1_2019_04_20T22_51_24.210/working/VLASS1.2.sb36458312.eb36595350.58593.54284034722_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t30.J235832+373000_P44904v1_2019_04_20T22_51_24.210/working
Start time
2020-01-01 06:32:14.783
End
2020-01-01 06:33:48.424
Duration
0:01:33.642
Note, WebLog generation is not included in the time.

CASA logs for stage 6