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 8.2525e-04 Jy/beam
minimum 1.2566e-04 Jy/beam
mean 2.0674e-04 Jy/beam
median 1.5422e-04 Jy/beam
sigma 1.0748e-04 Jy/beam
MAD rms 1.6171e-05 Jy/beam

RMS images

VLASS1.2.sb36478588.eb36498992.58563.30308221065_split.ms

VLASS1.2.ql.T15t17.J122316_193000.10.2048.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_T15t17.J122316+193000_P37081v1_2019_03_27T23_42_23.904/working/VLASS1.2.sb36478588.eb36498992.58563.30308221065_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t17.J122316+193000_P37081v1_2019_03_27T23_42_23.904/working
Start time
2019-03-28 23:29:35.816
End
2019-03-28 23:31:21.083
Duration
0:01:45.267
Note, WebLog generation is not included in the time.

CASA logs for stage 6