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 7.2804e-04 Jy/beam
minimum 1.2613e-04 Jy/beam
mean 2.0814e-04 Jy/beam
median 1.6069e-04 Jy/beam
sigma 9.5627e-05 Jy/beam
MAD rms 2.7199e-05 Jy/beam

RMS images

VLASS1.2.sb36437873.eb36581239.58589.510090717595_split.ms

VLASS1.2.ql.T09t27.J174611_073000.10.2048.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_T09t27.J174611-073000_P44194v1_2019_05_03T16_09_42.215/working/VLASS1.2.sb36437873.eb36581239.58589.510090717595_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T09t27.J174611-073000_P44194v1_2019_05_03T16_09_42.215/working
Start time
2019-05-08 16:04:55.377
End
2019-05-08 16:06:49.345
Duration
0:01:53.968
Note, WebLog generation is not included in the time.

CASA logs for stage 6