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 5.8538e-04 Jy/beam
minimum 1.0916e-04 Jy/beam
mean 1.8201e-04 Jy/beam
median 1.5914e-04 Jy/beam
sigma 7.6028e-05 Jy/beam
MAD rms 4.5733e-05 Jy/beam

RMS images

VLASS1.2.sb36474059.eb36491204.58561.31710584491_split.ms

VLASS1.2.ql.T22t14.J135748_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_T22t14.J135748+443000_P38014v1_2019_10_11T19_23_12.823/working/VLASS1.2.sb36474059.eb36491204.58561.31710584491_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T22t14.J135748+443000_P38014v1_2019_10_11T19_23_12.823/working
Start time
2019-10-12 20:52:18.713
End
2019-10-12 20:53:44.373
Duration
0:01:25.660
Note, WebLog generation is not included in the time.

CASA logs for stage 6