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 1.0222e-03 Jy/beam
minimum 1.4296e-04 Jy/beam
mean 2.2539e-04 Jy/beam
median 1.7183e-04 Jy/beam
sigma 1.0856e-04 Jy/beam
MAD rms 1.9702e-05 Jy/beam

RMS images

VLASS1.2.sb36757663.eb36826436.58665.30243090278_split.ms

VLASS1.2.ql.T05t04.J021042_213000.10.2048.v1.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_T05t04.J021042-213000_P53778v1_2019_07_22T22_55_16.201/working/VLASS1.2.sb36757663.eb36826436.58665.30243090278_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T05t04.J021042-213000_P53778v1_2019_07_22T22_55_16.201/working
Start time
2019-07-29 18:18:36.624
End
2019-07-29 18:20:28.088
Duration
0:01:51.463
Note, WebLog generation is not included in the time.

CASA logs for stage 6