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 4.8469e-02 Jy/beam
minimum 1.4576e-04 Jy/beam
mean 5.5532e-04 Jy/beam
median 2.1048e-04 Jy/beam
sigma 1.7188e-03 Jy/beam
MAD rms 6.7920e-05 Jy/beam

RMS images

VLASS1.2.sb36758729.eb36826063.58663.33838615741_split.ms

VLASS1.2.ql.T05t05.J024210_233000.10.2048.v2.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T05t05.J024210-233000_P53946v2_2019_07_19T20_13_02.098/working/VLASS1.2.sb36758729.eb36826063.58663.33838615741_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T05t05.J024210-233000_P53946v2_2019_07_19T20_13_02.098/working
Start time
2019-07-22 03:20:22.642
End
2019-07-22 03:22:29.843
Duration
0:02:07.201
Note, WebLog generation is not included in the time.

CASA logs for stage 6