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 6.6328e-04 Jy/beam
minimum 1.2105e-04 Jy/beam
mean 1.9141e-04 Jy/beam
median 1.4876e-04 Jy/beam
sigma 8.8429e-05 Jy/beam
MAD rms 1.6123e-05 Jy/beam

RMS images

VLASS1.2.sb36452026.eb36490802.58560.43470678241_split.ms

VLASS1.2.ql.T13t25.J162624_103000.10.2048.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_T13t25.J162624+103000_P36495v1_2019_03_27T23_33_23.396/working/VLASS1.2.sb36452026.eb36490802.58560.43470678241_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T13t25.J162624+103000_P36495v1_2019_03_27T23_33_23.396/working
Start time
2019-03-28 23:52:08.215
End
2019-03-28 23:53:51.022
Duration
0:01:42.807
Note, WebLog generation is not included in the time.

CASA logs for stage 6