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 6.1054e-04 Jy/beam
minimum 1.1321e-04 Jy/beam
mean 1.7823e-04 Jy/beam
median 1.3512e-04 Jy/beam
sigma 8.5221e-05 Jy/beam
MAD rms 1.3532e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t25.J180217_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_T18t25.J180217+293000_P50399v1_2019_06_26T15_22_50.008/working/VLASS1.2.sb36674765.eb36802005.58655.17007922454_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t25.J180217+293000_P50399v1_2019_06_26T15_22_50.008/working
Start time
2019-06-27 23:00:11.890
End
2019-06-27 23:02:08.668
Duration
0:01:56.778
Note, WebLog generation is not included in the time.

CASA logs for stage 6