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 6.9774e-04 Jy/beam
minimum 1.2268e-04 Jy/beam
mean 2.1469e-04 Jy/beam
median 1.6687e-04 Jy/beam
sigma 9.7809e-05 Jy/beam
MAD rms 3.7977e-05 Jy/beam

RMS images

VLASS1.1.sb34894726.eb34973224.58148.30825349537_split.ms

VLASS1.1.ql.T07t16.J103838_153000.10.2048.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_T07t16.J103838-153000_P22180v2_2018_01_30T22_54_54.033/working/VLASS1.1.sb34894726.eb34973224.58148.30825349537_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T07t16.J103838-153000_P22180v2_2018_01_30T22_54_54.033/working
Start time
2021-05-15 21:14:31.303
End
2021-05-15 21:15:33.054
Duration
0:01:01.750
Note, WebLog generation is not included in the time.

CASA logs for stage 6