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 6.4091e-04 Jy/beam
minimum 1.2025e-04 Jy/beam
mean 1.8630e-04 Jy/beam
median 1.4359e-04 Jy/beam
sigma 9.0355e-05 Jy/beam
MAD rms 1.3028e-05 Jy/beam

RMS images

VLASS1.2.sb36674136.eb36677242.58625.28268025463_split.ms

VLASS1.2.ql.T18t30.J215151_293000.10.2048.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_T18t30.J215151+293000_P50318v1_2019_06_03T22_59_45.003/working/VLASS1.2.sb36674136.eb36677242.58625.28268025463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t30.J215151+293000_P50318v1_2019_06_03T22_59_45.003/working
Start time
2019-06-05 08:06:52.120
End
2019-06-05 08:09:05.774
Duration
0:02:13.654
Note, WebLog generation is not included in the time.

CASA logs for stage 6