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 1.2737e-03 Jy/beam
minimum 1.0276e-04 Jy/beam
mean 1.6688e-04 Jy/beam
median 1.2445e-04 Jy/beam
sigma 8.8194e-05 Jy/beam
MAD rms 1.4156e-05 Jy/beam

RMS images

VLASS1.1.sb35045706.eb35051188.58162.78700490741_split.ms

VLASS1.1.ql.T03t35.J224218_303000.10.2048.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_T03t35.J224218-303000_P26260v2_2018_02_13T19_00_05.100/working/VLASS1.1.sb35045706.eb35051188.58162.78700490741_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T03t35.J224218-303000_P26260v2_2018_02_13T19_00_05.100/working
Start time
2021-06-27 17:47:38.281
End
2021-06-27 17:49:00.607
Duration
0:01:22.326
Note, WebLog generation is not included in the time.

CASA logs for stage 6