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 7.7640e-04 Jy/beam
minimum 1.1223e-04 Jy/beam
mean 1.8087e-04 Jy/beam
median 1.3928e-04 Jy/beam
sigma 9.0023e-05 Jy/beam
MAD rms 1.8004e-05 Jy/beam

RMS images

VLASS1.2.sb36529284.eb36595213.58592.50811275463_split.ms

VLASS1.2.ql.T20t28.J215345_383000.10.2048.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_T20t28.J215345+383000_P40529v1_2019_05_04T18_08_07.564/working/VLASS1.2.sb36529284.eb36595213.58592.50811275463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t28.J215345+383000_P40529v1_2019_05_04T18_08_07.564/working
Start time
2019-05-09 03:08:22.625
End
2019-05-09 03:10:42.667
Duration
0:02:20.041
Note, WebLog generation is not included in the time.

CASA logs for stage 6