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 7.0529e-04 Jy/beam
minimum 1.1433e-04 Jy/beam
mean 1.8494e-04 Jy/beam
median 1.4725e-04 Jy/beam
sigma 8.0446e-05 Jy/beam
MAD rms 2.2308e-05 Jy/beam

RMS images

VLASS1.1.sb34748147.eb34823345.58130.14045111111_split.ms

VLASS1.1.ql.T11t12.J075800_023000.10.2048.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_T11t12.J075800+023000_P19978v2_2018_01_12T21_39_32.550/working/VLASS1.1.sb34748147.eb34823345.58130.14045111111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T11t12.J075800+023000_P19978v2_2018_01_12T21_39_32.550/working
Start time
2021-05-06 14:01:06.618
End
2021-05-06 14:02:24.139
Duration
0:01:17.521
Note, WebLog generation is not included in the time.

CASA logs for stage 6