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 6.1457e-04 Jy/beam
minimum 1.2253e-04 Jy/beam
mean 2.1936e-04 Jy/beam
median 1.8939e-04 Jy/beam
sigma 8.6666e-05 Jy/beam
MAD rms 5.1313e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T21t16.J155936_423000.10.2048.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_T21t16.J155936+423000_P39390v1_2019_10_21T22_01_55.709/working/VLASS1.2.sb36491285.eb36526783.58570.391316724534_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t16.J155936+423000_P39390v1_2019_10_21T22_01_55.709/working
Start time
2019-10-22 13:47:53.978
End
2019-10-22 13:49:12.861
Duration
0:01:18.883
Note, WebLog generation is not included in the time.

CASA logs for stage 6