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 6.0138e-04 Jy/beam
minimum 1.1213e-04 Jy/beam
mean 1.7450e-04 Jy/beam
median 1.3269e-04 Jy/beam
sigma 8.0490e-05 Jy/beam
MAD rms 1.3392e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T22t23.J221439_473000.10.2048.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.J221439+473000_P49916v1_2019_05_28T23_09_16.843/working/VLASS1.2.sb36651475.eb36670581.58622.36553387731_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T22t23.J221439+473000_P49916v1_2019_05_28T23_09_16.843/working
Start time
2019-05-31 16:21:24.309
End
2019-05-31 16:23:14.901
Duration
0:01:50.592
Note, WebLog generation is not included in the time.

CASA logs for stage 6