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 7.8502e-04 Jy/beam
minimum 1.6467e-04 Jy/beam
mean 2.5818e-04 Jy/beam
median 2.1293e-04 Jy/beam
sigma 1.0376e-04 Jy/beam
MAD rms 3.2357e-05 Jy/beam

RMS images

VLASS2.1.sb38447583.eb38589602.59083.73025677083_split.ms

VLASS2.1.ql.T11t18.J115401_023000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T11t18.J115401+023000_P56670v1_2020_08_22T23_01_47.189/working/VLASS2.1.sb38447583.eb38589602.59083.73025677083_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T11t18.J115401+023000_P56670v1_2020_08_22T23_01_47.189/working
Start time
2020-09-03 18:49:26.440
End
2020-09-03 18:51:10.251
Duration
0:01:43.811
Note, WebLog generation is not included in the time.

CASA logs for stage 6