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 1.3963e-03 Jy/beam
minimum 1.1742e-04 Jy/beam
mean 2.0425e-04 Jy/beam
median 1.5424e-04 Jy/beam
sigma 1.0867e-04 Jy/beam
MAD rms 3.5045e-05 Jy/beam

RMS images

VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms

VLASS1.2.ql.T18t25.J182926_283000.10.2048.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_T18t25.J182926+283000_P50395v1_2019_06_28T18_01_40.407/working/VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t25.J182926+283000_P50395v1_2019_06_28T18_01_40.407/working
Start time
2019-06-30 10:02:41.450
End
2019-06-30 10:03:48.544
Duration
0:01:07.094
Note, WebLog generation is not included in the time.

CASA logs for stage 6