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 5.8491e-04 Jy/beam
minimum 1.0994e-04 Jy/beam
mean 1.7323e-04 Jy/beam
median 1.3393e-04 Jy/beam
sigma 8.0579e-05 Jy/beam
MAD rms 1.3894e-05 Jy/beam

RMS images

VLASS1.2.sb36651475.eb36670581.58622.36553387731_split.ms

VLASS1.2.ql.T21t23.J221908_433000.10.2048.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_T21t23.J221908+433000_P49873v1_2019_05_28T23_07_34.162/working/VLASS1.2.sb36651475.eb36670581.58622.36553387731_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t23.J221908+433000_P49873v1_2019_05_28T23_07_34.162/working
Start time
2019-06-01 18:32:40.033
End
2019-06-01 18:35:06.982
Duration
0:02:26.949
Note, WebLog generation is not included in the time.

CASA logs for stage 6