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 6.7557e-04 Jy/beam
minimum 1.1546e-04 Jy/beam
mean 1.7984e-04 Jy/beam
median 1.3819e-04 Jy/beam
sigma 8.7416e-05 Jy/beam
MAD rms 1.1909e-05 Jy/beam

RMS images

VLASS1.2.sb36675323.eb36772845.58643.26662539352_split.ms

VLASS1.2.ql.T18t31.J224126_293000.10.2048.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_T18t31.J224126+293000_P50646v1_2019_06_14T22_00_46.364/working/VLASS1.2.sb36675323.eb36772845.58643.26662539352_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t31.J224126+293000_P50646v1_2019_06_14T22_00_46.364/working
Start time
2019-06-16 16:59:33.436
End
2019-06-16 17:01:34.551
Duration
0:02:01.115
Note, WebLog generation is not included in the time.

CASA logs for stage 6