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 6.7218e-04 Jy/beam
minimum 1.0789e-04 Jy/beam
mean 1.8335e-04 Jy/beam
median 1.4323e-04 Jy/beam
sigma 8.4803e-05 Jy/beam
MAD rms 2.0755e-05 Jy/beam

RMS images

VLASS1.1.sb34746916.eb34812604.58123.11002827546_split.ms

VLASS1.1.ql.T11t10.J060200_013000.10.2048.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_T11t10.J060200+013000_P19834v2_2018_01_05T00_07_54.373/working/VLASS1.1.sb34746916.eb34812604.58123.11002827546_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T11t10.J060200+013000_P19834v2_2018_01_05T00_07_54.373/working
Start time
2021-04-29 13:56:51.900
End
2021-04-29 13:58:08.299
Duration
0:01:16.399
Note, WebLog generation is not included in the time.

CASA logs for stage 6