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 7.5728e-04 Jy/beam
minimum 1.1942e-04 Jy/beam
mean 1.9827e-04 Jy/beam
median 1.4964e-04 Jy/beam
sigma 9.9784e-05 Jy/beam
MAD rms 1.6773e-05 Jy/beam

RMS images

VLASS1.2.sb36685904.eb36847422.58671.580943877314_split.ms

VLASS1.2.ql.T01t19.J090743_393000.10.2048.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_T01t19.J090743-393000_P52151v1_2019_07_22T20_06_02.112/working/VLASS1.2.sb36685904.eb36847422.58671.580943877314_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T01t19.J090743-393000_P52151v1_2019_07_22T20_06_02.112/working
Start time
2019-07-27 03:23:17.778
End
2019-07-27 03:25:22.046
Duration
0:02:04.268
Note, WebLog generation is not included in the time.

CASA logs for stage 6