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 7.5942e-04 Jy/beam
minimum 1.2860e-04 Jy/beam
mean 2.1013e-04 Jy/beam
median 1.5896e-04 Jy/beam
sigma 1.0207e-04 Jy/beam
MAD rms 2.1826e-05 Jy/beam

RMS images

VLASS1.2.sb36437873.eb36581239.58589.510090717595_split.ms

VLASS1.2.ql.T09t30.J192602_073000.10.2048.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_T09t30.J192602-073000_P44149v1_2019_04_30T22_05_32.824/working/VLASS1.2.sb36437873.eb36581239.58589.510090717595_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T09t30.J192602-073000_P44149v1_2019_04_30T22_05_32.824/working
Start time
2019-05-03 17:32:21.236
End
2019-05-03 17:34:20.190
Duration
0:01:58.954
Note, WebLog generation is not included in the time.

CASA logs for stage 6