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 6.4060e-04 Jy/beam
minimum 1.0534e-04 Jy/beam
mean 1.8025e-04 Jy/beam
median 1.3409e-04 Jy/beam
sigma 9.2672e-05 Jy/beam
MAD rms 2.1263e-05 Jy/beam

RMS images

VLASS1.1.sb34898226.eb35042893.58162.29820586806_split.ms

VLASS1.1.ql.T03t26.J171807_283000.10.2048.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_T03t26.J171807-283000_P25051v2_2018_02_13T17_26_51.931/working/VLASS1.1.sb34898226.eb35042893.58162.29820586806_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T03t26.J171807-283000_P25051v2_2018_02_13T17_26_51.931/working
Start time
2021-08-22 17:02:19.312
End
2021-08-22 17:03:23.903
Duration
0:01:04.591
Note, WebLog generation is not included in the time.

CASA logs for stage 6