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 5.8884e-04 Jy/beam
minimum 1.0976e-04 Jy/beam
mean 1.8493e-04 Jy/beam
median 1.3492e-04 Jy/beam
sigma 9.3717e-05 Jy/beam
MAD rms 1.7958e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T20t28.J214821_363000.10.2048.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.J214821+363000_P40508v1_2019_05_09T14_21_11.219/working/VLASS1.2.sb36529284.eb36595213.58592.50811275463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t28.J214821+363000_P40508v1_2019_05_09T14_21_11.219/working
Start time
2019-05-10 13:07:42.887
End
2019-05-10 13:09:03.309
Duration
0:01:20.422
Note, WebLog generation is not included in the time.

CASA logs for stage 6