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 6.3871e-04 Jy/beam
minimum 1.2064e-04 Jy/beam
mean 1.9149e-04 Jy/beam
median 1.4529e-04 Jy/beam
sigma 9.2221e-05 Jy/beam
MAD rms 1.4418e-05 Jy/beam

RMS images

VLASS2.1.sb38610763.eb38659643.59111.9147512037_split.ms

VLASS2.1.ql.T20t19.J145218_393000.10.2048.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_T20t19.J145218+393000_P70083v1_2020_09_19T18_18_34.907/working/VLASS2.1.sb38610763.eb38659643.59111.9147512037_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T20t19.J145218+393000_P70083v1_2020_09_19T18_18_34.907/working
Start time
2020-10-04 07:42:13.594
End
2020-10-04 07:43:39.603
Duration
0:01:26.009
Note, WebLog generation is not included in the time.

CASA logs for stage 6