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 7.8234e-04 Jy/beam
minimum 1.2991e-04 Jy/beam
mean 2.0971e-04 Jy/beam
median 1.6198e-04 Jy/beam
sigma 1.0576e-04 Jy/beam
MAD rms 1.6028e-05 Jy/beam

RMS images

VLASS1.2.sb36530723.eb36540184.58571.90369828704_split.ms

VLASS1.2.ql.T15t10.J065118_183000.10.2048.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_T15t10.J065118+183000_P41550v1_2019_04_02T22_01_14.611/working/VLASS1.2.sb36530723.eb36540184.58571.90369828704_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t10.J065118+183000_P41550v1_2019_04_02T22_01_14.611/working
Start time
2019-04-04 11:28:23.361
End
2019-04-04 11:30:30.473
Duration
0:02:07.112
Note, WebLog generation is not included in the time.

CASA logs for stage 6