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 8.2881e-04 Jy/beam
minimum 1.3598e-04 Jy/beam
mean 2.1602e-04 Jy/beam
median 1.6974e-04 Jy/beam
sigma 1.0308e-04 Jy/beam
MAD rms 1.9486e-05 Jy/beam

RMS images

VLASS1.2.sb36454866.eb36490672.58559.499279571755_split.ms

VLASS1.2.ql.T12t28.J182207_063000.10.2048.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_T12t28.J182207+063000_P36740v1_2019_03_27T23_25_41.697/working/VLASS1.2.sb36454866.eb36490672.58559.499279571755_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T12t28.J182207+063000_P36740v1_2019_03_27T23_25_41.697/working
Start time
2019-03-28 22:21:46.401
End
2019-03-28 22:23:47.483
Duration
0:02:01.082
Note, WebLog generation is not included in the time.

CASA logs for stage 6