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 7.2501e-04 Jy/beam
minimum 1.1608e-04 Jy/beam
mean 1.7614e-04 Jy/beam
median 1.3511e-04 Jy/beam
sigma 8.5639e-05 Jy/beam
MAD rms 1.0613e-05 Jy/beam

RMS images

VLASS1.2.sb36518823.eb36595674.58595.435916689814_split.ms

VLASS1.2.ql.T15t29.J210618_183000.10.2048.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_T15t29.J210618+183000_P43831v1_2019_05_12T19_50_26.444/working/VLASS1.2.sb36518823.eb36595674.58595.435916689814_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t29.J210618+183000_P43831v1_2019_05_12T19_50_26.444/working
Start time
2019-05-15 06:51:29.434
End
2019-05-15 06:53:42.055
Duration
0:02:12.621
Note, WebLog generation is not included in the time.

CASA logs for stage 6