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 7.1055e-04 Jy/beam
minimum 1.1216e-04 Jy/beam
mean 2.0803e-04 Jy/beam
median 1.6751e-04 Jy/beam
sigma 1.0411e-04 Jy/beam
MAD rms 5.2496e-05 Jy/beam

RMS images

VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms

VLASS1.2.ql.T18t10.J072817_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_T18t10.J072817+303000_P41908v1_2019_12_10T16_16_20.475/working/VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t10.J072817+303000_P41908v1_2019_12_10T16_16_20.475/working
Start time
2019-12-11 07:39:52.545
End
2019-12-11 07:41:03.089
Duration
0:01:10.544
Note, WebLog generation is not included in the time.

CASA logs for stage 6