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 6.8871e-04 Jy/beam
minimum 1.1996e-04 Jy/beam
mean 1.9013e-04 Jy/beam
median 1.4520e-04 Jy/beam
sigma 9.5647e-05 Jy/beam
MAD rms 1.7287e-05 Jy/beam

RMS images

VLASS1.2.sb36461910.eb36513329.58566.766115624996_split.ms

VLASS1.2.ql.T16t05.J031909_203000.10.2048.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_T16t05.J031909+203000_P37181v1_2019_04_01T22_46_22.425/working/VLASS1.2.sb36461910.eb36513329.58566.766115624996_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T16t05.J031909+203000_P37181v1_2019_04_01T22_46_22.425/working
Start time
2019-04-03 18:08:49.888
End
2019-04-03 18:11:11.947
Duration
0:02:22.059
Note, WebLog generation is not included in the time.

CASA logs for stage 6