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 7.4369e-04 Jy/beam
minimum 1.0900e-04 Jy/beam
mean 1.9599e-04 Jy/beam
median 1.6501e-04 Jy/beam
sigma 8.9145e-05 Jy/beam
MAD rms 5.0830e-05 Jy/beam

RMS images

VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms

VLASS1.2.ql.T18t08.J051718_303000.10.2048.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_T18t08.J051718+303000_P37889v1_2019_10_21T21_25_16.074/working/VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t08.J051718+303000_P37889v1_2019_10_21T21_25_16.074/working
Start time
2019-10-23 00:37:45.361
End
2019-10-23 00:39:29.433
Duration
0:01:44.073
Note, WebLog generation is not included in the time.

CASA logs for stage 6