6. Make RMS Uncertainty Images

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 6.9959e-04 Jy/beam
minimum 1.1636e-04 Jy/beam
mean 2.0344e-04 Jy/beam
median 1.5035e-04 Jy/beam
sigma 1.0373e-04 Jy/beam
MAD rms 2.7183e-05 Jy/beam

RMS images

VLASS1.1.sb34919742.eb34993475.58152.22067622685_split.ms

VLASS1.1.ql.T02t25.J122938_353000.10.2048.v2.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T02t25.J122938-353000_P22463v2_2018_02_03T22_51_12.001/working/VLASS1.1.sb34919742.eb34993475.58152.22067622685_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T02t25.J122938-353000_P22463v2_2018_02_03T22_51_12.001/working
Start time
2021-05-13 22:38:36.980
End
2021-05-13 22:39:34.950
Duration
0:00:57.970
Note, WebLog generation is not included in the time.

CASA logs for stage 6