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 6.5882e-04 Jy/beam
minimum 1.1431e-04 Jy/beam
mean 1.8581e-04 Jy/beam
median 1.4210e-04 Jy/beam
sigma 9.3970e-05 Jy/beam
MAD rms 1.6614e-05 Jy/beam

RMS images

VLASS1.2.sb36526854.eb36581717.58589.84345299768_split.ms

VLASS1.2.ql.T17t13.J092841_253000.10.2048.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_T17t13.J092841+253000_P40689v1_2019_05_01T15_04_52.833/working/VLASS1.2.sb36526854.eb36581717.58589.84345299768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t13.J092841+253000_P40689v1_2019_05_01T15_04_52.833/working
Start time
2019-05-04 18:14:51.450
End
2019-05-04 18:16:53.871
Duration
0:02:02.422
Note, WebLog generation is not included in the time.

CASA logs for stage 6