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 6.0581e-04 Jy/beam
minimum 1.1096e-04 Jy/beam
mean 1.7311e-04 Jy/beam
median 1.3407e-04 Jy/beam
sigma 8.2221e-05 Jy/beam
MAD rms 1.3503e-05 Jy/beam

RMS images

VLASS1.2.sb36624415.eb36765605.58641.29728032407_split.ms

VLASS1.2.ql.T19t30.J235232_333000.10.2048.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_T19t30.J235232+333000_P48766v1_2019_06_14T18_19_06.891/working/VLASS1.2.sb36624415.eb36765605.58641.29728032407_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T19t30.J235232+333000_P48766v1_2019_06_14T18_19_06.891/working
Start time
2019-06-16 10:18:59.551
End
2019-06-16 10:20:39.628
Duration
0:01:40.077
Note, WebLog generation is not included in the time.

CASA logs for stage 6