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 6.6339e-04 Jy/beam
minimum 1.2730e-04 Jy/beam
mean 2.2237e-04 Jy/beam
median 1.6373e-04 Jy/beam
sigma 1.1159e-04 Jy/beam
MAD rms 2.9806e-05 Jy/beam

RMS images

VLASS1.2.sb36754487.eb36826246.58664.70754203704_split.ms

VLASS1.2.ql.T04t18.J115942_243000.10.2048.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_T04t18.J115942-243000_P54607v1_2019_07_09T18_54_26.517/working/VLASS1.2.sb36754487.eb36826246.58664.70754203704_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T04t18.J115942-243000_P54607v1_2019_07_09T18_54_26.517/working
Start time
2019-07-12 21:18:58.092
End
2019-07-12 21:20:08.052
Duration
0:01:09.959
Note, WebLog generation is not included in the time.

CASA logs for stage 6