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 6.9941e-04 Jy/beam
minimum 1.2435e-04 Jy/beam
mean 1.9599e-04 Jy/beam
median 1.4669e-04 Jy/beam
sigma 1.0029e-04 Jy/beam
MAD rms 1.2611e-05 Jy/beam

RMS images

VLASS2.1.sb38759130.eb38879035.59154.06567945602_split.ms

VLASS2.1.ql.T05t02.J005909_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/VLASS2.1_T05t02.J005909-203000_P76575v1_2020_11_01T22_56_22.848/working/VLASS2.1.sb38759130.eb38879035.59154.06567945602_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T05t02.J005909-203000_P76575v1_2020_11_01T22_56_22.848/working
Start time
2020-11-23 23:01:13.155
End
2020-11-23 23:02:37.565
Duration
0:01:24.410
Note, WebLog generation is not included in the time.

CASA logs for stage 6