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 9.5732e-04 Jy/beam
minimum 1.8338e-04 Jy/beam
mean 2.9832e-04 Jy/beam
median 2.3583e-04 Jy/beam
sigma 1.2404e-04 Jy/beam
MAD rms 3.3341e-05 Jy/beam

RMS images

VLASS2.1.sb38610195.eb38638028.59101.102248043986_split.ms

VLASS2.1.ql.T19t23.J181237_353000.10.2048.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_T19t23.J181237+353000_P70043v1_2020_09_09T20_13_10.492/working/VLASS2.1.sb38610195.eb38638028.59101.102248043986_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T19t23.J181237+353000_P70043v1_2020_09_09T20_13_10.492/working
Start time
2020-09-18 04:47:37.625
End
2020-09-18 04:48:55.575
Duration
0:01:17.951
Note, WebLog generation is not included in the time.

CASA logs for stage 6