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 5.9000e-04 Jy/beam
minimum 1.1069e-04 Jy/beam
mean 1.7508e-04 Jy/beam
median 1.3191e-04 Jy/beam
sigma 8.5481e-05 Jy/beam
MAD rms 1.2968e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t04.J024959_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.J024959+313000_P37866v1_2019_04_01T22_28_03.993/working/VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t04.J024959+313000_P37866v1_2019_04_01T22_28_03.993/working
Start time
2019-04-03 03:53:50.127
End
2019-04-03 03:55:39.961
Duration
0:01:49.835
Note, WebLog generation is not included in the time.

CASA logs for stage 6