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 7.7900e-04 Jy/beam
minimum 1.4422e-04 Jy/beam
mean 2.3045e-04 Jy/beam
median 1.8252e-04 Jy/beam
sigma 1.0044e-04 Jy/beam
MAD rms 2.7953e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T12t25.J161804_053000.10.2048.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.J161804+053000_P36523v1_2019_03_29T20_00_27.594/working/VLASS1.2.sb36452026.eb36490802.58560.43470678241_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T12t25.J161804+053000_P36523v1_2019_03_29T20_00_27.594/working
Start time
2019-04-01 06:32:20.799
End
2019-04-01 06:34:11.644
Duration
0:01:50.844
Note, WebLog generation is not included in the time.

CASA logs for stage 6