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 6.1932e-04 Jy/beam
minimum 1.0912e-04 Jy/beam
mean 1.9281e-04 Jy/beam
median 1.6512e-04 Jy/beam
sigma 8.3686e-05 Jy/beam
MAD rms 5.9654e-05 Jy/beam

RMS images

VLASS1.2.sb36484370.eb36574402.58585.3477416088_split.ms

VLASS1.2.ql.T15t22.J154706_193000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t22.J154706+193000_P38767v1_2019_12_09T17_38_17.929/working/VLASS1.2.sb36484370.eb36574402.58585.3477416088_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t22.J154706+193000_P38767v1_2019_12_09T17_38_17.929/working
Start time
2019-12-10 10:26:38.662
End
2019-12-10 10:27:41.486
Duration
0:01:02.824
Note, WebLog generation is not included in the time.

CASA logs for stage 6