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 5.8308e-04 Jy/beam
minimum 1.1381e-04 Jy/beam
mean 1.7502e-04 Jy/beam
median 1.3526e-04 Jy/beam
sigma 8.2558e-05 Jy/beam
MAD rms 1.2116e-05 Jy/beam

RMS images

VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms

VLASS1.2.ql.T18t25.J181132_303000.10.2048.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_T18t25.J181132+303000_P50411v1_2019_06_26T15_23_50.151/working/VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t25.J181132+303000_P50411v1_2019_06_26T15_23_50.151/working
Start time
2019-06-28 08:53:42.842
End
2019-06-28 08:55:40.494
Duration
0:01:57.652
Note, WebLog generation is not included in the time.

CASA logs for stage 6