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 6.1253e-04 Jy/beam
minimum 1.1173e-04 Jy/beam
mean 1.8510e-04 Jy/beam
median 1.3910e-04 Jy/beam
sigma 8.9850e-05 Jy/beam
MAD rms 1.6015e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t25.J184317_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_T18t25.J184317+303000_P50418v1_2019_06_26T15_24_25.804/working/VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t25.J184317+303000_P50418v1_2019_06_26T15_24_25.804/working
Start time
2019-06-28 01:37:09.965
End
2019-06-28 01:38:41.776
Duration
0:01:31.811
Note, WebLog generation is not included in the time.

CASA logs for stage 6