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 8.9850e-04 Jy/beam
minimum 1.0082e-04 Jy/beam
mean 1.8197e-04 Jy/beam
median 1.3122e-04 Jy/beam
sigma 1.0138e-04 Jy/beam
MAD rms 2.5311e-05 Jy/beam

RMS images

VLASS1.1.sb34552309.eb34700380.58074.807198912036_split.ms

VLASS1.1.ql.T16t24.J175847_203000.10.2048.v3.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_T16t24.J175847+203000_P13711v3_2017_11_17T22_11_23.884/working/VLASS1.1.sb34552309.eb34700380.58074.807198912036_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T16t24.J175847+203000_P13711v3_2017_11_17T22_11_23.884/working
Start time
2020-06-10 11:15:25.003
End
2020-06-10 11:16:06.051
Duration
0:00:41.048
Note, WebLog generation is not included in the time.

CASA logs for stage 6