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 7.9926e-04 Jy/beam
minimum 1.3383e-04 Jy/beam
mean 2.1143e-04 Jy/beam
median 1.6620e-04 Jy/beam
sigma 9.2932e-05 Jy/beam
MAD rms 1.7398e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T08t21.J133813_093000.10.2048.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.J133813-093000_P35526v1_2019_03_13T21_32_22.038/working/VLASS1.2.sb36407335.eb36457033.58548.350781851856_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T08t21.J133813-093000_P35526v1_2019_03_13T21_32_22.038/working
Start time
2019-03-15 01:40:25.596
End
2019-03-15 01:42:34.778
Duration
0:02:09.182
Note, WebLog generation is not included in the time.

CASA logs for stage 6