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 6.3759e-04 Jy/beam
minimum 1.1942e-04 Jy/beam
mean 1.9636e-04 Jy/beam
median 1.4888e-04 Jy/beam
sigma 9.3329e-05 Jy/beam
MAD rms 2.2412e-05 Jy/beam

RMS images

VLASS1.1.sb34692336.eb34811412.58121.33896026621_split.ms

VLASS1.1.ql.T12t18.J115802_043000.10.2048.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_T12t18.J115802+043000_P18355v2_2018_01_03T22_23_39.244/working/VLASS1.1.sb34692336.eb34811412.58121.33896026621_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T12t18.J115802+043000_P18355v2_2018_01_03T22_23_39.244/working
Start time
2021-05-07 16:35:07.547
End
2021-05-07 16:36:11.552
Duration
0:01:04.005
Note, WebLog generation is not included in the time.

CASA logs for stage 6