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 7.7044e-04 Jy/beam
minimum 1.1058e-04 Jy/beam
mean 1.9017e-04 Jy/beam
median 1.3972e-04 Jy/beam
sigma 9.6407e-05 Jy/beam
MAD rms 2.2767e-05 Jy/beam

RMS images

VLASS1.2.sb36663230.eb36777152.58647.27793965278_split.ms

VLASS1.2.ql.T18t28.J201718_303000.10.2048.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_T18t28.J201718+303000_P50201v1_2019_12_02T18_53_12.314/working/VLASS1.2.sb36663230.eb36777152.58647.27793965278_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t28.J201718+303000_P50201v1_2019_12_02T18_53_12.314/working
Start time
2019-12-05 00:03:32.427
End
2019-12-05 00:04:25.671
Duration
0:00:53.245
Note, WebLog generation is not included in the time.

CASA logs for stage 6