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 5.7536e-04 Jy/beam
minimum 1.1459e-04 Jy/beam
mean 1.8029e-04 Jy/beam
median 1.3978e-04 Jy/beam
sigma 8.2500e-05 Jy/beam
MAD rms 1.5366e-05 Jy/beam

RMS images

VLASS1.2.sb36459161.eb36630310.58605.46792393518_split.ms

VLASS1.2.ql.T23t24.J234543_493000.10.2048.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_T23t24.J234543+493000_P44388v1_2019_05_17T23_18_15.900/working/VLASS1.2.sb36459161.eb36630310.58605.46792393518_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t24.J234543+493000_P44388v1_2019_05_17T23_18_15.900/working
Start time
2019-05-20 05:48:13.963
End
2019-05-20 05:50:24.914
Duration
0:02:10.952
Note, WebLog generation is not included in the time.

CASA logs for stage 6