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 7.1929e-04 Jy/beam
minimum 1.2409e-04 Jy/beam
mean 2.1857e-04 Jy/beam
median 1.8911e-04 Jy/beam
sigma 8.7505e-05 Jy/beam
MAD rms 5.9390e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t08.J055804_293000.10.2048.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.J055804+293000_P37888v1_2019_10_21T21_25_18.363/working/VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t08.J055804+293000_P37888v1_2019_10_21T21_25_18.363/working
Start time
2019-10-23 04:24:28.631
End
2019-10-23 04:26:08.183
Duration
0:01:39.551
Note, WebLog generation is not included in the time.

CASA logs for stage 6