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 7.1458e-04 Jy/beam
minimum 1.0704e-04 Jy/beam
mean 1.7706e-04 Jy/beam
median 1.3029e-04 Jy/beam
sigma 9.2906e-05 Jy/beam
MAD rms 1.3713e-05 Jy/beam

RMS images

VLASS2.2.sb40457323.eb40504141.59493.006917453706_split.ms

VLASS2.2.ql.T13t28.J183816_103000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.2_T13t28.J183816+103000_P82415v1_2021_10_06T20_12_29.747/working/VLASS2.2.sb40457323.eb40504141.59493.006917453706_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.2_T13t28.J183816+103000_P82415v1_2021_10_06T20_12_29.747/working
Start time
2021-10-12 16:30:54.113
End
2021-10-12 16:32:04.230
Duration
0:01:10.118
Note, WebLog generation is not included in the time.

CASA logs for stage 6