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 7.7225e-04 Jy/beam
minimum 1.2535e-04 Jy/beam
mean 2.0198e-04 Jy/beam
median 1.5069e-04 Jy/beam
sigma 1.0278e-04 Jy/beam
MAD rms 1.6054e-05 Jy/beam

RMS images

VLASS2.1.sb38538105.eb38585498.59082.21856813657_split.ms

VLASS2.1.ql.T26t18.J232522_613000.10.2048.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_T26t18.J232522+613000_P65613v1_2020_08_21T23_09_54.913/working/VLASS2.1.sb38538105.eb38585498.59082.21856813657_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T26t18.J232522+613000_P65613v1_2020_08_21T23_09_54.913/working
Start time
2020-08-28 22:34:36.661
End
2020-08-28 22:35:56.342
Duration
0:01:19.681
Note, WebLog generation is not included in the time.

CASA logs for stage 6