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 6.3715e-04 Jy/beam
minimum 1.1772e-04 Jy/beam
mean 1.8993e-04 Jy/beam
median 1.4505e-04 Jy/beam
sigma 9.1470e-05 Jy/beam
MAD rms 1.6570e-05 Jy/beam

RMS images

VLASS1.2.sb36470480.eb36511597.58565.708401296295_split.ms

VLASS1.2.ql.T17t02.J011327_243000.10.2048.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_T17t02.J011327+243000_P37319v1_2019_04_08T19_08_49.677/working/VLASS1.2.sb36470480.eb36511597.58565.708401296295_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t02.J011327+243000_P37319v1_2019_04_08T19_08_49.677/working
Start time
2019-04-10 05:15:21.086
End
2019-04-10 05:16:56.764
Duration
0:01:35.679
Note, WebLog generation is not included in the time.

CASA logs for stage 6