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 6.6367e-04 Jy/beam
minimum 1.2562e-04 Jy/beam
mean 1.9752e-04 Jy/beam
median 1.5340e-04 Jy/beam
sigma 8.7518e-05 Jy/beam
MAD rms 1.6173e-05 Jy/beam

RMS images

VLASS1.2.sb36488226.eb36546988.58575.44941939815_split.ms

VLASS1.2.ql.T14t29.J191103_153000.10.2048.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_T14t29.J191103+153000_P38256v1_2019_05_01T14_58_51.543/working/VLASS1.2.sb36488226.eb36546988.58575.44941939815_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t29.J191103+153000_P38256v1_2019_05_01T14_58_51.543/working
Start time
2019-05-03 19:47:28.261
End
2019-05-03 19:49:38.653
Duration
0:02:10.393
Note, WebLog generation is not included in the time.

CASA logs for stage 6