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 8.2566e-04 Jy/beam
minimum 1.2938e-04 Jy/beam
mean 2.3523e-04 Jy/beam
median 1.9823e-04 Jy/beam
sigma 1.0145e-04 Jy/beam
MAD rms 6.2427e-05 Jy/beam

RMS images

VLASS1.2.sb36494144.eb36600323.58596.320760752315_split.ms

VLASS1.2.ql.T11t23.J151801_033000.10.2048.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_T11t23.J151801+033000_P38953v1_2019_12_10T17_03_01.837/working/VLASS1.2.sb36494144.eb36600323.58596.320760752315_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T11t23.J151801+033000_P38953v1_2019_12_10T17_03_01.837/working
Start time
2019-12-11 04:19:24.296
End
2019-12-11 04:20:32.674
Duration
0:01:08.378
Note, WebLog generation is not included in the time.

CASA logs for stage 6