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 6.5228e-04 Jy/beam
minimum 1.2354e-04 Jy/beam
mean 1.9183e-04 Jy/beam
median 1.4741e-04 Jy/beam
sigma 8.9997e-05 Jy/beam
MAD rms 1.4035e-05 Jy/beam

RMS images

VLASS1.2.sb36508448.eb36679671.58626.40843943287_split.ms

VLASS1.2.ql.T23t23.J221514_493000.10.2048.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_T23t23.J221514+493000_P43379v1_2019_06_04T23_06_45.147/working/VLASS1.2.sb36508448.eb36679671.58626.40843943287_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t23.J221514+493000_P43379v1_2019_06_04T23_06_45.147/working
Start time
2019-06-06 19:39:01.747
End
2019-06-06 19:41:07.631
Duration
0:02:05.884
Note, WebLog generation is not included in the time.

CASA logs for stage 6