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 7.8544e-04 Jy/beam
minimum 1.3905e-04 Jy/beam
mean 2.4367e-04 Jy/beam
median 1.8032e-04 Jy/beam
sigma 1.3090e-04 Jy/beam
MAD rms 3.5039e-05 Jy/beam

RMS images

VLASS2.1.sb38756914.eb38895852.59158.79950653935_split.ms

VLASS2.1.ql.T03t29.J184217_293000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T03t29.J184217-293000_P76184v1_2020_11_05T22_05_41.032/working/VLASS2.1.sb38756914.eb38895852.59158.79950653935_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T03t29.J184217-293000_P76184v1_2020_11_05T22_05_41.032/working
Start time
2020-12-22 07:34:35.904
End
2020-12-22 07:35:30.036
Duration
0:00:54.132
Note, WebLog generation is not included in the time.

CASA logs for stage 6