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 6.8911e-04 Jy/beam
minimum 1.3551e-04 Jy/beam
mean 2.2138e-04 Jy/beam
median 1.7057e-04 Jy/beam
sigma 1.0032e-04 Jy/beam
MAD rms 2.1013e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T09t33.J213808_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_T09t33.J213808-073000_P44112v1_2019_04_30T22_04_12.743/working/VLASS1.2.sb36437873.eb36581239.58589.510090717595_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T09t33.J213808-073000_P44112v1_2019_04_30T22_04_12.743/working
Start time
2019-05-02 17:22:53.792
End
2019-05-02 17:24:59.659
Duration
0:02:05.867
Note, WebLog generation is not included in the time.

CASA logs for stage 6