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 6.7690e-04 Jy/beam
minimum 1.2089e-04 Jy/beam
mean 1.9839e-04 Jy/beam
median 1.5062e-04 Jy/beam
sigma 9.9693e-05 Jy/beam
MAD rms 1.9432e-05 Jy/beam

RMS images

VLASS2.1.sb38504727.eb38659863.59113.352947384265_split.ms

VLASS2.1.ql.T13t13.J083438_113000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T13t13.J083438+113000_P61586v1_2020_09_21T18_17_47.717/working/VLASS2.1.sb38504727.eb38659863.59113.352947384265_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T13t13.J083438+113000_P61586v1_2020_09_21T18_17_47.717/working
Start time
2020-10-18 20:35:46.485
End
2020-10-18 20:37:03.411
Duration
0:01:16.926
Note, WebLog generation is not included in the time.

CASA logs for stage 6