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 1.1693e-03 Jy/beam
minimum 1.1345e-04 Jy/beam
mean 1.9396e-04 Jy/beam
median 1.4922e-04 Jy/beam
sigma 9.5942e-05 Jy/beam
MAD rms 2.9804e-05 Jy/beam

RMS images

VLASS1.2.sb36468339.eb36560182.58580.68005592593_split.ms

VLASS1.2.ql.T18t07.J045539_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_T18t07.J045539+313000_P37822v1_2019_04_16T17_18_44.017/working/VLASS1.2.sb36468339.eb36560182.58580.68005592593_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t07.J045539+313000_P37822v1_2019_04_16T17_18_44.017/working
Start time
2019-04-19 17:41:13.985
End
2019-04-19 17:42:41.166
Duration
0:01:27.181
Note, WebLog generation is not included in the time.

CASA logs for stage 6