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 8.1933e-04 Jy/beam
minimum 1.2715e-04 Jy/beam
mean 1.9981e-04 Jy/beam
median 1.5447e-04 Jy/beam
sigma 8.9178e-05 Jy/beam
MAD rms 1.7481e-05 Jy/beam

RMS images

VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms

VLASS1.2.ql.T14t30.J193418_123000.10.2048.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_T14t30.J193418+123000_P38100v1_2019_04_04T22_34_10.793/working/VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t30.J193418+123000_P38100v1_2019_04_04T22_34_10.793/working
Start time
2019-04-06 13:18:03.403
End
2019-04-06 13:19:32.659
Duration
0:01:29.257
Note, WebLog generation is not included in the time.

CASA logs for stage 6