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 5.9689e-04 Jy/beam
minimum 1.1486e-04 Jy/beam
mean 1.7915e-04 Jy/beam
median 1.3531e-04 Jy/beam
sigma 8.8408e-05 Jy/beam
MAD rms 1.2533e-05 Jy/beam

RMS images

VLASS1.2.sb36458312.eb36595350.58593.54284034722_split.ms

VLASS1.2.ql.T20t30.J232918_363000.10.2048.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_T20t30.J232918+363000_P44888v1_2019_05_09T14_35_48.423/working/VLASS1.2.sb36458312.eb36595350.58593.54284034722_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t30.J232918+363000_P44888v1_2019_05_09T14_35_48.423/working
Start time
2019-05-11 06:00:43.515
End
2019-05-11 06:02:55.471
Duration
0:02:11.956
Note, WebLog generation is not included in the time.

CASA logs for stage 6