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 3.4040e-03 Jy/beam
minimum 1.1251e-04 Jy/beam
mean 2.1049e-04 Jy/beam
median 1.5049e-04 Jy/beam
sigma 1.4840e-04 Jy/beam
MAD rms 3.1640e-05 Jy/beam

RMS images

VLASS1.2.sb36617763.eb36631658.58606.046132268515_split.ms

VLASS1.2.ql.T20t11.J082818_393000.10.2048.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_T20t11.J082818+393000_P48536v1_2019_05_28T17_31_40.341/working/VLASS1.2.sb36617763.eb36631658.58606.046132268515_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t11.J082818+393000_P48536v1_2019_05_28T17_31_40.341/working
Start time
2019-06-03 01:57:30.100
End
2019-06-03 01:58:42.960
Duration
0:01:12.860
Note, WebLog generation is not included in the time.

CASA logs for stage 6