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 6.7358e-04 Jy/beam
minimum 1.1631e-04 Jy/beam
mean 1.9087e-04 Jy/beam
median 1.4283e-04 Jy/beam
sigma 9.8234e-05 Jy/beam
MAD rms 1.6364e-05 Jy/beam

RMS images

VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms

VLASS1.2.ql.T18t14.J101039_313000.10.2048.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_T18t14.J101039+313000_P41954v1_2019_05_12T19_59_22.200/working/VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t14.J101039+313000_P41954v1_2019_05_12T19_59_22.200/working
Start time
2019-05-14 21:22:04.502
End
2019-05-14 21:23:49.688
Duration
0:01:45.186
Note, WebLog generation is not included in the time.

CASA logs for stage 6