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 8.4604e-04 Jy/beam
minimum 1.1217e-04 Jy/beam
mean 1.8233e-04 Jy/beam
median 1.3875e-04 Jy/beam
sigma 9.1718e-05 Jy/beam
MAD rms 1.5974e-05 Jy/beam

RMS images

VLASS1.2.sb36617763.eb36631658.58606.046132268515_split.ms

VLASS1.2.ql.T20t11.J081231_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_T20t11.J081231+373000_P48513v1_2019_05_18T16_04_16.619/working/VLASS1.2.sb36617763.eb36631658.58606.046132268515_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t11.J081231+373000_P48513v1_2019_05_18T16_04_16.619/working
Start time
2019-05-20 23:54:52.086
End
2019-05-20 23:57:04.945
Duration
0:02:12.859
Note, WebLog generation is not included in the time.

CASA logs for stage 6