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 1.0196e-03 Jy/beam
minimum 1.1230e-04 Jy/beam
mean 1.8211e-04 Jy/beam
median 1.3699e-04 Jy/beam
sigma 9.2427e-05 Jy/beam
MAD rms 1.6324e-05 Jy/beam

RMS images

VLASS1.2.sb36663230.eb36777152.58647.27793965278_split.ms

VLASS1.2.ql.T18t32.J235804_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_T18t32.J235804+293000_P50240v1_2019_12_03T23_50_43.985/working/VLASS1.2.sb36663230.eb36777152.58647.27793965278_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t32.J235804+293000_P50240v1_2019_12_03T23_50_43.985/working
Start time
2019-12-04 23:44:31.176
End
2019-12-04 23:45:46.447
Duration
0:01:15.271
Note, WebLog generation is not included in the time.

CASA logs for stage 6