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 8.5442e-04 Jy/beam
minimum 1.3631e-04 Jy/beam
mean 2.3575e-04 Jy/beam
median 1.6941e-04 Jy/beam
sigma 1.2806e-04 Jy/beam
MAD rms 2.5019e-05 Jy/beam

RMS images

VLASS2.1.sb38498189.eb38518036.59051.15321533565_split.ms

VLASS2.1.ql.T11t29.J191800_003000.10.2048.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_T11t29.J191800+003000_P61177v1_2020_07_21T16_31_26.824/working/VLASS2.1.sb38498189.eb38518036.59051.15321533565_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T11t29.J191800+003000_P61177v1_2020_07_21T16_31_26.824/working
Start time
2020-08-07 21:49:37.884
End
2020-08-07 21:50:26.588
Duration
0:00:48.703
Note, WebLog generation is not included in the time.

CASA logs for stage 6