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 9.8552e-04 Jy/beam
minimum 1.1307e-04 Jy/beam
mean 1.8827e-04 Jy/beam
median 1.4040e-04 Jy/beam
sigma 9.9217e-05 Jy/beam
MAD rms 1.5017e-05 Jy/beam

RMS images

VLASS2.1.sb38751098.eb38840212.59147.84691032408_split.ms

VLASS2.1.ql.T01t42.J205250_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/VLASS2.1_T01t42.J205250-383000_P75943v1_2020_10_25T23_30_55.585/working/VLASS2.1.sb38751098.eb38840212.59147.84691032408_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T01t42.J205250-383000_P75943v1_2020_10_25T23_30_55.585/working
Start time
2020-12-02 15:58:29.699
End
2020-12-02 16:00:13.632
Duration
0:01:43.933
Note, WebLog generation is not included in the time.

CASA logs for stage 6