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 5.8828e-04 Jy/beam
minimum 1.0992e-04 Jy/beam
mean 1.7628e-04 Jy/beam
median 1.3583e-04 Jy/beam
sigma 8.1726e-05 Jy/beam
MAD rms 1.6294e-05 Jy/beam

RMS images

VLASS1.2.sb36651475.eb36670581.58622.36553387731_split.ms

VLASS1.2.ql.T21t23.J225449_403000.10.2048.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_T21t23.J225449+403000_P49844v1_2019_10_16T20_53_36.154/working/VLASS1.2.sb36651475.eb36670581.58622.36553387731_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t23.J225449+403000_P49844v1_2019_10_16T20_53_36.154/working
Start time
2019-10-17 23:15:51.867
End
2019-10-17 23:17:23.521
Duration
0:01:31.654
Note, WebLog generation is not included in the time.

CASA logs for stage 6