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 8.2936e-04 Jy/beam
minimum 1.5764e-04 Jy/beam
mean 2.5501e-04 Jy/beam
median 2.0267e-04 Jy/beam
sigma 1.1455e-04 Jy/beam
MAD rms 2.5499e-05 Jy/beam

RMS images

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

VLASS2.1.ql.T24t12.J111027_553000.10.2048.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.J111027+553000_P63361v1_2020_08_02T16_33_51.975/working/VLASS2.1.sb38520431.eb38554942.59063.924480127316_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T24t12.J111027+553000_P63361v1_2020_08_02T16_33_51.975/working
Start time
2020-10-01 16:47:53.711
End
2020-10-01 16:49:20.917
Duration
0:01:27.206
Note, WebLog generation is not included in the time.

CASA logs for stage 6