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 6.8568e-04 Jy/beam
minimum 1.3718e-04 Jy/beam
mean 2.2081e-04 Jy/beam
median 1.7027e-04 Jy/beam
sigma 9.8088e-05 Jy/beam
MAD rms 2.2690e-05 Jy/beam

RMS images

VLASS1.2.sb36730336.eb36770756.58641.97701479167_split.ms

VLASS1.2.ql.T08t14.J091810_083000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T08t14.J091810-083000_P51418v1_2019_11_25T16_40_32.355/working/VLASS1.2.sb36730336.eb36770756.58641.97701479167_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T08t14.J091810-083000_P51418v1_2019_11_25T16_40_32.355/working
Start time
2019-11-26 02:59:20.903
End
2019-11-26 03:00:30.687
Duration
0:01:09.784
Note, WebLog generation is not included in the time.

CASA logs for stage 6