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 6.4049e-04 Jy/beam
minimum 1.0943e-04 Jy/beam
mean 1.7325e-04 Jy/beam
median 1.3061e-04 Jy/beam
sigma 8.9737e-05 Jy/beam
MAD rms 1.0594e-05 Jy/beam

RMS images

VLASS1.2.sb36587627.eb36593858.58591.95807649306_split.ms

VLASS1.2.ql.T16t14.J095953_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_T16t14.J095953+203000_P46291v1_2019_05_02T23_41_40.814/working/VLASS1.2.sb36587627.eb36593858.58591.95807649306_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T16t14.J095953+203000_P46291v1_2019_05_02T23_41_40.814/working
Start time
2019-05-06 16:33:50.186
End
2019-05-06 16:36:21.398
Duration
0:02:31.211
Note, WebLog generation is not included in the time.

CASA logs for stage 6