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 8.2073e-04 Jy/beam
minimum 1.1093e-04 Jy/beam
mean 1.8013e-04 Jy/beam
median 1.3603e-04 Jy/beam
sigma 8.7569e-05 Jy/beam
MAD rms 1.7392e-05 Jy/beam

RMS images

VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms

VLASS1.2.ql.T18t04.J022159_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_T18t04.J022159+313000_P37860v1_2019_04_01T22_27_53.721/working/VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t04.J022159+313000_P37860v1_2019_04_01T22_27_53.721/working
Start time
2019-04-03 16:51:21.944
End
2019-04-03 16:53:09.470
Duration
0:01:47.526
Note, WebLog generation is not included in the time.

CASA logs for stage 6