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 7.9622e-04 Jy/beam
minimum 1.4103e-04 Jy/beam
mean 2.4165e-04 Jy/beam
median 1.8085e-04 Jy/beam
sigma 1.1878e-04 Jy/beam
MAD rms 2.7317e-05 Jy/beam

RMS images

VLASS1.2.sb36454866.eb36490672.58559.499279571755_split.ms

VLASS1.2.ql.T12t28.J181002_053000.10.2048.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_T12t28.J181002+053000_P36727v1_2019_03_29T17_20_43.431/working/VLASS1.2.sb36454866.eb36490672.58559.499279571755_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T12t28.J181002+053000_P36727v1_2019_03_29T17_20_43.431/working
Start time
2019-03-30 01:37:31.054
End
2019-03-30 01:38:45.960
Duration
0:01:14.906
Note, WebLog generation is not included in the time.

CASA logs for stage 6