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 6.0606e-04 Jy/beam
minimum 1.1512e-04 Jy/beam
mean 1.8390e-04 Jy/beam
median 1.4146e-04 Jy/beam
sigma 8.7681e-05 Jy/beam
MAD rms 1.6149e-05 Jy/beam

RMS images

VLASS1.2.sb36491855.eb36574404.58585.53016267361_split.ms

VLASS1.2.ql.T25t15.J193504_573000.10.2048.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_T25t15.J193504+573000_P39272v1_2019_04_18T18_05_04.975/working/VLASS1.2.sb36491855.eb36574404.58585.53016267361_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T25t15.J193504+573000_P39272v1_2019_04_18T18_05_04.975/working
Start time
2019-04-19 19:53:37.158
End
2019-04-19 19:55:16.671
Duration
0:01:39.513
Note, WebLog generation is not included in the time.

CASA logs for stage 6