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 6.4937e-04 Jy/beam
minimum 1.1818e-04 Jy/beam
mean 2.0055e-04 Jy/beam
median 1.7198e-04 Jy/beam
sigma 8.5558e-05 Jy/beam
MAD rms 5.1736e-05 Jy/beam

RMS images

VLASS1.2.sb36491285.eb36526783.58570.391316724534_split.ms

VLASS1.2.ql.T22t16.J150246_443000.10.2048.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_T22t16.J150246+443000_P39311v1_2019_10_21T22_01_26.821/working/VLASS1.2.sb36491285.eb36526783.58570.391316724534_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T22t16.J150246+443000_P39311v1_2019_10_21T22_01_26.821/working
Start time
2019-10-22 22:05:57.595
End
2019-10-22 22:07:48.787
Duration
0:01:51.192
Note, WebLog generation is not included in the time.

CASA logs for stage 6