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 6.0180e-04 Jy/beam
minimum 1.0710e-04 Jy/beam
mean 1.7830e-04 Jy/beam
median 1.3288e-04 Jy/beam
sigma 8.6106e-05 Jy/beam
MAD rms 1.9823e-05 Jy/beam

RMS images

VLASS1.2.sb36537755.eb36576550.58586.16342928241_split.ms

VLASS1.2.ql.T18t11.J080915_303000.10.2048.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_T18t11.J080915+303000_P45718v1_2019_04_23T21_14_16.501/working/VLASS1.2.sb36537755.eb36576550.58586.16342928241_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t11.J080915+303000_P45718v1_2019_04_23T21_14_16.501/working
Start time
2019-04-24 08:17:16.884
End
2019-04-24 08:18:29.595
Duration
0:01:12.710
Note, WebLog generation is not included in the time.

CASA logs for stage 6