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 8.4617e-04 Jy/beam
minimum 1.1712e-04 Jy/beam
mean 2.0332e-04 Jy/beam
median 1.4781e-04 Jy/beam
sigma 1.1040e-04 Jy/beam
MAD rms 1.9906e-05 Jy/beam

RMS images

VLASS1.2.sb36717844.eb36839665.58669.28246069445_split.ms

VLASS1.2.ql.T01t40.J193730_373000.10.2048.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_T01t40.J193730-373000_P52731v1_2019_07_29T17_43_52.074/working/VLASS1.2.sb36717844.eb36839665.58669.28246069445_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T01t40.J193730-373000_P52731v1_2019_07_29T17_43_52.074/working
Start time
2019-08-01 05:09:52.534
End
2019-08-01 05:11:18.807
Duration
0:01:26.273
Note, WebLog generation is not included in the time.

CASA logs for stage 6