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 6.8424e-04 Jy/beam
minimum 1.0610e-04 Jy/beam
mean 1.7703e-04 Jy/beam
median 1.3129e-04 Jy/beam
sigma 9.3845e-05 Jy/beam
MAD rms 1.6897e-05 Jy/beam

RMS images

VLASS1.1.sb34552309.eb34700380.58074.807198912036_split.ms

VLASS1.1.ql.T16t20.J141710_233000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T16t20.J141710+233000_P13690v2_2017_11_17T17_17_58.827/working/VLASS1.1.sb34552309.eb34700380.58074.807198912036_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T16t20.J141710+233000_P13690v2_2017_11_17T17_17_58.827/working
Start time
2020-04-16 15:34:51.168
End
2020-04-16 15:35:53.900
Duration
0:01:02.732
Note, WebLog generation is not included in the time.

CASA logs for stage 6