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 6.9696e-04 Jy/beam
minimum 1.3093e-04 Jy/beam
mean 2.1326e-04 Jy/beam
median 1.6826e-04 Jy/beam
sigma 9.4006e-05 Jy/beam
MAD rms 2.6134e-05 Jy/beam

RMS images

VLASS1.2.sb36407335.eb36457033.58548.350781851856_split.ms

VLASS1.2.ql.T08t21.J133810_083000.10.2048.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_T08t21.J133810-083000_P35536v1_2019_03_13T21_33_37.724/working/VLASS1.2.sb36407335.eb36457033.58548.350781851856_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T08t21.J133810-083000_P35536v1_2019_03_13T21_33_37.724/working
Start time
2019-03-15 19:21:24.038
End
2019-03-15 19:23:17.157
Duration
0:01:53.119
Note, WebLog generation is not included in the time.

CASA logs for stage 6