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 7.9283e-04 Jy/beam
minimum 1.1951e-04 Jy/beam
mean 1.9612e-04 Jy/beam
median 1.4570e-04 Jy/beam
sigma 1.0509e-04 Jy/beam
MAD rms 1.5424e-05 Jy/beam

RMS images

VLASS1.2.sb36714658.eb36863414.58674.19097365741_split.ms

VLASS1.2.ql.T02t01.J001212_353000.10.2048.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_T02t01.J001212-353000_P52368v1_2019_07_29T23_37_12.606/working/VLASS1.2.sb36714658.eb36863414.58674.19097365741_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T02t01.J001212-353000_P52368v1_2019_07_29T23_37_12.606/working
Start time
2019-08-03 14:24:07.187
End
2019-08-03 14:26:26.609
Duration
0:02:19.422
Note, WebLog generation is not included in the time.

CASA logs for stage 6