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 5.2700e-04 Jy/beam
minimum 1.0523e-04 Jy/beam
mean 1.6334e-04 Jy/beam
median 1.2620e-04 Jy/beam
sigma 7.6253e-05 Jy/beam
MAD rms 1.1926e-05 Jy/beam

RMS images

VLASS1.2.sb36507182.eb36649330.58612.33337462963_split.ms

VLASS1.2.ql.T23t21.J201533_503000.10.2048.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_T23t21.J201533+503000_P43209v1_2019_05_28T20_56_45.969/working/VLASS1.2.sb36507182.eb36649330.58612.33337462963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t21.J201533+503000_P43209v1_2019_05_28T20_56_45.969/working
Start time
2019-05-31 08:25:13.089
End
2019-05-31 08:27:30.292
Duration
0:02:17.203
Note, WebLog generation is not included in the time.

CASA logs for stage 6