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 6.4377e-04 Jy/beam
minimum 1.0634e-04 Jy/beam
mean 1.8225e-04 Jy/beam
median 1.3625e-04 Jy/beam
sigma 8.8182e-05 Jy/beam
MAD rms 2.4214e-05 Jy/beam

RMS images

VLASS1.1.sb34900388.eb35074823.58165.26784681713_split.ms

VLASS1.1.ql.T04t19.J123951_253000.10.2048.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_T04t19.J123951-253000_P24735v2_2018_02_16T23_44_18.588/working/VLASS1.1.sb34900388.eb35074823.58165.26784681713_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T04t19.J123951-253000_P24735v2_2018_02_16T23_44_18.588/working
Start time
2021-07-31 20:04:45.273
End
2021-07-31 20:05:47.397
Duration
0:01:02.123
Note, WebLog generation is not included in the time.

CASA logs for stage 6