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 1.8057e-03 Jy/beam
minimum 1.3819e-04 Jy/beam
mean 2.2624e-04 Jy/beam
median 1.7308e-04 Jy/beam
sigma 1.1053e-04 Jy/beam
MAD rms 2.2287e-05 Jy/beam

RMS images

VLASS1.2.sb36404986.eb36465932.58552.531894976855_split.ms

VLASS1.2.ql.T08t28.J183017_083000.10.2048.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_T08t28.J183017-083000_P35785v1_2019_04_05T17_18_03.012/working/VLASS1.2.sb36404986.eb36465932.58552.531894976855_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T08t28.J183017-083000_P35785v1_2019_04_05T17_18_03.012/working
Start time
2019-04-07 06:58:45.222
End
2019-04-07 07:00:36.507
Duration
0:01:51.285
Note, WebLog generation is not included in the time.

CASA logs for stage 6