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 6.7784e-04 Jy/beam
minimum 1.1751e-04 Jy/beam
mean 1.8694e-04 Jy/beam
median 1.4051e-04 Jy/beam
sigma 9.4447e-05 Jy/beam
MAD rms 1.2724e-05 Jy/beam

RMS images

VLASS2.1.sb38613707.eb38659860.59113.15663519676_split.ms

VLASS2.1.ql.T20t25.J191924_363000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T20t25.J191924+363000_P70213v1_2020_09_21T20_34_15.409/working/VLASS2.1.sb38613707.eb38659860.59113.15663519676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T20t25.J191924+363000_P70213v1_2020_09_21T20_34_15.409/working
Start time
2020-10-04 04:17:12.737
End
2020-10-04 04:18:36.378
Duration
0:01:23.641
Note, WebLog generation is not included in the time.

CASA logs for stage 6