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 6.9675e-04 Jy/beam
minimum 1.2069e-04 Jy/beam
mean 2.0128e-04 Jy/beam
median 1.5582e-04 Jy/beam
sigma 9.7049e-05 Jy/beam
MAD rms 2.2697e-05 Jy/beam

RMS images

VLASS1.2.sb36492430.eb36542481.58573.39361230324_split.ms

VLASS1.2.ql.T15t20.J142524_163000.10.2048.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_T15t20.J142524+163000_P39138v1_2019_04_04T15_19_29.054/working/VLASS1.2.sb36492430.eb36542481.58573.39361230324_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t20.J142524+163000_P39138v1_2019_04_04T15_19_29.054/working
Start time
2019-04-05 13:26:05.257
End
2019-04-05 13:28:07.743
Duration
0:02:02.485
Note, WebLog generation is not included in the time.

CASA logs for stage 6