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 6.6711e-04 Jy/beam
minimum 1.2541e-04 Jy/beam
mean 2.0853e-04 Jy/beam
median 1.5456e-04 Jy/beam
sigma 1.0227e-04 Jy/beam
MAD rms 2.1908e-05 Jy/beam

RMS images

VLASS1.2.sb36452026.eb36490802.58560.43470678241_split.ms

VLASS1.2.ql.T13t25.J161007_093000.10.2048.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_T13t25.J161007+093000_P36481v1_2019_03_28T19_52_54.118/working/VLASS1.2.sb36452026.eb36490802.58560.43470678241_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T13t25.J161007+093000_P36481v1_2019_03_28T19_52_54.118/working
Start time
2019-03-29 04:33:07.503
End
2019-03-29 04:34:20.592
Duration
0:01:13.089
Note, WebLog generation is not included in the time.

CASA logs for stage 6