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 5.8165e-04 Jy/beam
minimum 1.1362e-04 Jy/beam
mean 1.8103e-04 Jy/beam
median 1.3643e-04 Jy/beam
sigma 8.7028e-05 Jy/beam
MAD rms 1.4218e-05 Jy/beam

RMS images

VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms

VLASS1.2.ql.T18t25.J183830_283000.10.2048.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_T18t25.J183830+283000_P50397v1_2019_06_26T15_22_44.503/working/VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t25.J183830+283000_P50397v1_2019_06_26T15_22_44.503/working
Start time
2019-06-27 17:52:29.984
End
2019-06-27 17:54:08.728
Duration
0:01:38.743
Note, WebLog generation is not included in the time.

CASA logs for stage 6