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 6.5972e-04 Jy/beam
minimum 1.1267e-04 Jy/beam
mean 2.0809e-04 Jy/beam
median 1.7088e-04 Jy/beam
sigma 9.8765e-05 Jy/beam
MAD rms 5.6314e-05 Jy/beam

RMS images

VLASS1.2.sb36470480.eb36511597.58565.708401296295_split.ms

VLASS1.2.ql.T17t06.J042716_263000.10.2048.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_T17t06.J042716+263000_P37388v1_2019_10_16T20_20_02.677/working/VLASS1.2.sb36470480.eb36511597.58565.708401296295_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t06.J042716+263000_P37388v1_2019_10_16T20_20_02.677/working
Start time
2019-10-17 13:26:09.450
End
2019-10-17 13:27:16.741
Duration
0:01:07.291
Note, WebLog generation is not included in the time.

CASA logs for stage 6