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 1.2816e-03 Jy/beam
minimum 1.1571e-04 Jy/beam
mean 1.9610e-04 Jy/beam
median 1.4806e-04 Jy/beam
sigma 1.0346e-04 Jy/beam
MAD rms 2.0243e-05 Jy/beam

RMS images

VLASS1.2.sb36527441.eb36595314.58592.866473229165_split.ms

VLASS1.2.ql.T17t14.J101840_273000.10.2048.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_T17t14.J101840+273000_P40802v1_2019_05_05T21_22_08.616/working/VLASS1.2.sb36527441.eb36595314.58592.866473229165_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t14.J101840+273000_P40802v1_2019_05_05T21_22_08.616/working
Start time
2019-05-09 00:10:32.671
End
2019-05-09 00:12:27.604
Duration
0:01:54.933
Note, WebLog generation is not included in the time.

CASA logs for stage 6