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 7.0617e-04 Jy/beam
minimum 1.3905e-04 Jy/beam
mean 2.4048e-04 Jy/beam
median 2.0752e-04 Jy/beam
sigma 9.8068e-05 Jy/beam
MAD rms 6.1958e-05 Jy/beam

RMS images

VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms

VLASS1.2.ql.T18t13.J094317_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_T18t13.J094317+303000_P41826v1_2019_04_20T23_19_20.917/working/VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t13.J094317+303000_P41826v1_2019_04_20T23_19_20.917/working
Start time
2020-01-01 19:45:23.192
End
2020-01-01 19:46:59.839
Duration
0:01:36.647
Note, WebLog generation is not included in the time.

CASA logs for stage 6