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 6.7188e-04 Jy/beam
minimum 1.2049e-04 Jy/beam
mean 2.0046e-04 Jy/beam
median 1.5311e-04 Jy/beam
sigma 9.8088e-05 Jy/beam
MAD rms 2.1825e-05 Jy/beam

RMS images

VLASS1.2.sb36674136.eb36677242.58625.28268025463_split.ms

VLASS1.2.ql.T18t30.J215639_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_T18t30.J215639+313000_P50339v1_2019_06_03T23_02_22.892/working/VLASS1.2.sb36674136.eb36677242.58625.28268025463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t30.J215639+313000_P50339v1_2019_06_03T23_02_22.892/working
Start time
2019-06-05 22:57:13.634
End
2019-06-05 22:59:18.813
Duration
0:02:05.179
Note, WebLog generation is not included in the time.

CASA logs for stage 6