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 9.0380e-04 Jy/beam
minimum 1.2629e-04 Jy/beam
mean 2.0197e-04 Jy/beam
median 1.5473e-04 Jy/beam
sigma 9.8464e-05 Jy/beam
MAD rms 1.8867e-05 Jy/beam

RMS images

VLASS2.1.sb38597432.eb38627615.59094.07999482639_split.ms

VLASS2.1.ql.T29t07.J181751_743000.10.2048.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_T29t07.J181751+743000_P69422v1_2020_09_02T17_00_46.945/working/VLASS2.1.sb38597432.eb38627615.59094.07999482639_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T29t07.J181751+743000_P69422v1_2020_09_02T17_00_46.945/working
Start time
2020-10-25 07:22:26.335
End
2020-10-25 07:23:58.095
Duration
0:01:31.759
Note, WebLog generation is not included in the time.

CASA logs for stage 6