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 6.5331e-04 Jy/beam
minimum 1.1985e-04 Jy/beam
mean 1.9623e-04 Jy/beam
median 1.4509e-04 Jy/beam
sigma 9.5417e-05 Jy/beam
MAD rms 2.0062e-05 Jy/beam

RMS images

VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms

VLASS1.2.ql.T23t09.J082654_483000.10.2048.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_T23t09.J082654+483000_P35335v1_2019_03_15T15_56_23.100/working/VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t09.J082654+483000_P35335v1_2019_03_15T15_56_23.100/working
Start time
2019-03-16 04:07:47.218
End
2019-03-16 04:08:57.177
Duration
0:01:09.959
Note, WebLog generation is not included in the time.

CASA logs for stage 6