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 6.0378e-04 Jy/beam
minimum 1.0302e-04 Jy/beam
mean 1.6028e-04 Jy/beam
median 1.2313e-04 Jy/beam
sigma 7.5927e-05 Jy/beam
MAD rms 1.1506e-05 Jy/beam

RMS images

VLASS1.2.sb36537755.eb36576550.58586.16342928241_split.ms

VLASS1.2.ql.T18t15.J104609_303000.10.2048.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_T18t15.J104609+303000_P45753v1_2019_04_22T20_39_57.331/working/VLASS1.2.sb36537755.eb36576550.58586.16342928241_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t15.J104609+303000_P45753v1_2019_04_22T20_39_57.331/working
Start time
2019-04-24 22:37:35.038
End
2019-04-24 22:39:36.414
Duration
0:02:01.376
Note, WebLog generation is not included in the time.

CASA logs for stage 6