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 8.1771e-04 Jy/beam
minimum 1.3657e-04 Jy/beam
mean 2.1811e-04 Jy/beam
median 1.7257e-04 Jy/beam
sigma 1.0029e-04 Jy/beam
MAD rms 1.9967e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T12t25.J161404_063000.10.2048.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_T12t25.J161404+063000_P36532v1_2019_03_27T23_35_57.782/working/VLASS1.2.sb36452026.eb36490802.58560.43470678241_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T12t25.J161404+063000_P36532v1_2019_03_27T23_35_57.782/working
Start time
2019-03-28 21:57:21.983
End
2019-03-28 21:59:22.702
Duration
0:02:00.719
Note, WebLog generation is not included in the time.

CASA logs for stage 6