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 7.4106e-04 Jy/beam
minimum 1.0883e-04 Jy/beam
mean 1.7046e-04 Jy/beam
median 1.3197e-04 Jy/beam
sigma 8.0185e-05 Jy/beam
MAD rms 1.2198e-05 Jy/beam

RMS images

VLASS1.2.sb36633416.eb36641475.58607.36298261574_split.ms

VLASS1.2.ql.T21t17.J160812_433000.10.2048.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_T21t17.J160812+433000_P49415v1_2019_05_07T22_39_01.723/working/VLASS1.2.sb36633416.eb36641475.58607.36298261574_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t17.J160812+433000_P49415v1_2019_05_07T22_39_01.723/working
Start time
2019-05-10 10:30:41.100
End
2019-05-10 10:32:48.690
Duration
0:02:07.590
Note, WebLog generation is not included in the time.

CASA logs for stage 6