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 6.2288e-04 Jy/beam
minimum 1.1253e-04 Jy/beam
mean 1.7509e-04 Jy/beam
median 1.3769e-04 Jy/beam
sigma 7.8581e-05 Jy/beam
MAD rms 1.4354e-05 Jy/beam

RMS images

VLASS1.2.sb36487638.eb36576920.58588.434619479165_split.ms

VLASS1.2.ql.T14t28.J181833_143000.10.2048.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_T14t28.J181833+143000_P38325v1_2019_04_29T01_49_10.336/working/VLASS1.2.sb36487638.eb36576920.58588.434619479165_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t28.J181833+143000_P38325v1_2019_04_29T01_49_10.336/working
Start time
2019-05-01 18:05:18.182
End
2019-05-01 18:07:55.072
Duration
0:02:36.890
Note, WebLog generation is not included in the time.

CASA logs for stage 6