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 1.1999e-03 Jy/beam
minimum 1.2253e-04 Jy/beam
mean 2.0102e-04 Jy/beam
median 1.5473e-04 Jy/beam
sigma 9.5853e-05 Jy/beam
MAD rms 2.1330e-05 Jy/beam

RMS images

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

VLASS2.1.ql.T02t38.J183224_343000.10.2048.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_T02t38.J183224-343000_P75912v1_2020_10_25T23_30_54.337/working/VLASS2.1.sb38751098.eb38840212.59147.84691032408_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T02t38.J183224-343000_P75912v1_2020_10_25T23_30_54.337/working
Start time
2020-11-29 14:41:27.902
End
2020-11-29 14:42:50.126
Duration
0:01:22.225
Note, WebLog generation is not included in the time.

CASA logs for stage 6