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 6.9115e-04 Jy/beam
minimum 1.1348e-04 Jy/beam
mean 1.8319e-04 Jy/beam
median 1.3663e-04 Jy/beam
sigma 9.4041e-05 Jy/beam
MAD rms 1.5705e-05 Jy/beam

RMS images

VLASS1.2.sb36587627.eb36593858.58591.95807649306_split.ms

VLASS1.2.ql.T16t14.J102526_203000.10.2048.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_T16t14.J102526+203000_P46297v1_2019_04_18T20_05_47.364/working/VLASS1.2.sb36587627.eb36593858.58591.95807649306_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T16t14.J102526+203000_P46297v1_2019_04_18T20_05_47.364/working
Start time
2019-12-26 01:38:31.292
End
2019-12-26 01:40:24.617
Duration
0:01:53.325
Note, WebLog generation is not included in the time.

CASA logs for stage 6