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 7.0800e-04 Jy/beam
minimum 1.0911e-04 Jy/beam
mean 1.7838e-04 Jy/beam
median 1.3468e-04 Jy/beam
sigma 8.7585e-05 Jy/beam
MAD rms 1.6932e-05 Jy/beam

RMS images

VLASS1.1.sb34725237.eb34739672.58079.98035050926_split.ms

VLASS1.1.ql.T08t33.J212201_083000.10.2048.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_T08t33.J212201-083000_P18826v2_2017_11_22T17_16_47.461/working/VLASS1.1.sb34725237.eb34739672.58079.98035050926_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T08t33.J212201-083000_P18826v2_2017_11_22T17_16_47.461/working
Start time
2021-02-11 09:49:05.586
End
2021-02-11 09:50:13.514
Duration
0:01:07.928
Note, WebLog generation is not included in the time.

CASA logs for stage 6