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 9.1596e-04 Jy/beam
minimum 1.5211e-04 Jy/beam
mean 2.6605e-04 Jy/beam
median 2.1928e-04 Jy/beam
sigma 1.1913e-04 Jy/beam
MAD rms 4.5126e-05 Jy/beam

RMS images

VLASS1.2.sb36407335.eb36457033.58548.350781851856_split.ms

VLASS1.2.ql.T08t19.J122212_083000.10.2048.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_T08t19.J122212-083000_P35497v1_2019_03_12T15_59_12.894/working/VLASS1.2.sb36407335.eb36457033.58548.350781851856_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T08t19.J122212-083000_P35497v1_2019_03_12T15_59_12.894/working
Start time
2019-03-13 05:50:42.797
End
2019-03-13 05:52:36.368
Duration
0:01:53.571
Note, WebLog generation is not included in the time.

CASA logs for stage 6