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 6.8603e-04 Jy/beam
minimum 1.2436e-04 Jy/beam
mean 2.1283e-04 Jy/beam
median 1.6044e-04 Jy/beam
sigma 1.0791e-04 Jy/beam
MAD rms 2.7489e-05 Jy/beam

RMS images

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

VLASS2.1.ql.T02t38.J185918_333000.10.2048.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.J185918-333000_P75925v1_2020_10_25T23_30_55.163/working/VLASS2.1.sb38751098.eb38840212.59147.84691032408_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T02t38.J185918-333000_P75925v1_2020_10_25T23_30_55.163/working
Start time
2020-11-28 13:28:23.712
End
2020-11-28 13:29:28.788
Duration
0:01:05.077
Note, WebLog generation is not included in the time.

CASA logs for stage 6