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 6.9542e-04 Jy/beam
minimum 1.0856e-04 Jy/beam
mean 1.7481e-04 Jy/beam
median 1.3580e-04 Jy/beam
sigma 8.3522e-05 Jy/beam
MAD rms 1.9692e-05 Jy/beam

RMS images

VLASS1.2.sb36651475.eb36670581.58622.36553387731_split.ms

VLASS1.2.ql.T22t23.J225249_443000.10.2048.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_T22t23.J225249+443000_P49890v1_2019_10_16T20_56_17.911/working/VLASS1.2.sb36651475.eb36670581.58622.36553387731_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T22t23.J225249+443000_P49890v1_2019_10_16T20_56_17.911/working
Start time
2019-10-18 14:45:45.688
End
2019-10-18 14:47:26.697
Duration
0:01:41.009
Note, WebLog generation is not included in the time.

CASA logs for stage 6