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 6.1627e-04 Jy/beam
minimum 1.2041e-04 Jy/beam
mean 1.8807e-04 Jy/beam
median 1.4811e-04 Jy/beam
sigma 8.2109e-05 Jy/beam
MAD rms 1.5826e-05 Jy/beam

RMS images

VLASS1.2.sb36412510.eb36580932.58589.12203866898_split.ms

VLASS1.2.ql.T09t19.J121404_063000.10.2048.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_T09t19.J121404-063000_P40193v1_2019_04_29T23_19_49.067/working/VLASS1.2.sb36412510.eb36580932.58589.12203866898_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T09t19.J121404-063000_P40193v1_2019_04_29T23_19_49.067/working
Start time
2019-05-02 22:01:43.518
End
2019-05-02 22:04:16.896
Duration
0:02:33.378
Note, WebLog generation is not included in the time.

CASA logs for stage 6