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 9.0393e-04 Jy/beam
minimum 1.8241e-04 Jy/beam
mean 2.8117e-04 Jy/beam
median 2.2405e-04 Jy/beam
sigma 1.1716e-04 Jy/beam
MAD rms 2.5588e-05 Jy/beam

RMS images

VLASS2.1.sb38520431.eb38554942.59063.924480127316_split.ms

VLASS2.1.ql.T24t12.J110958_533000.10.2048.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_T24t12.J110958+533000_P63342v1_2020_08_02T16_33_45.530/working/VLASS2.1.sb38520431.eb38554942.59063.924480127316_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T24t12.J110958+533000_P63342v1_2020_08_02T16_33_45.530/working
Start time
2020-10-01 20:58:51.499
End
2020-10-01 21:00:30.537
Duration
0:01:39.038
Note, WebLog generation is not included in the time.

CASA logs for stage 6