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 6.9639e-04 Jy/beam
minimum 1.2018e-04 Jy/beam
mean 1.8905e-04 Jy/beam
median 1.4280e-04 Jy/beam
sigma 1.0253e-04 Jy/beam
MAD rms 1.3045e-05 Jy/beam

RMS images

VLASS1.2.sb36587074.eb36595657.58594.95816284722_split.ms

VLASS1.2.ql.T16t13.J093208_213000.10.2048.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_T16t13.J093208+213000_P46216v1_2019_05_10T23_50_43.371/working/VLASS1.2.sb36587074.eb36595657.58594.95816284722_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T16t13.J093208+213000_P46216v1_2019_05_10T23_50_43.371/working
Start time
2019-05-14 08:48:34.992
End
2019-05-14 08:51:03.769
Duration
0:02:28.777
Note, WebLog generation is not included in the time.

CASA logs for stage 6