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 7.5960e-04 Jy/beam
minimum 1.1014e-04 Jy/beam
mean 1.9166e-04 Jy/beam
median 1.6037e-04 Jy/beam
sigma 8.8233e-05 Jy/beam
MAD rms 4.9040e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t04.J021718_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_T18t04.J021718+303000_P37849v1_2019_10_21T21_24_56.989/working/VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t04.J021718+303000_P37849v1_2019_10_21T21_24_56.989/working
Start time
2019-10-23 00:31:12.068
End
2019-10-23 00:33:04.203
Duration
0:01:52.135
Note, WebLog generation is not included in the time.

CASA logs for stage 6