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 6.0303e-04 Jy/beam
minimum 1.1752e-04 Jy/beam
mean 1.8712e-04 Jy/beam
median 1.4227e-04 Jy/beam
sigma 8.9843e-05 Jy/beam
MAD rms 1.4039e-05 Jy/beam

RMS images

VLASS1.2.sb36730934.eb36873193.58676.875373206014_split.ms

VLASS1.2.ql.T02t29.J142113_323000.10.2048.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_T02t29.J142113-323000_P52823v1_2019_08_02T18_20_10.693/working/VLASS1.2.sb36730934.eb36873193.58676.875373206014_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T02t29.J142113-323000_P52823v1_2019_08_02T18_20_10.693/working
Start time
2019-08-07 14:58:06.159
End
2019-08-07 15:00:28.910
Duration
0:02:22.751
Note, WebLog generation is not included in the time.

CASA logs for stage 6