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 6.0127e-04 Jy/beam
minimum 1.1281e-04 Jy/beam
mean 1.7533e-04 Jy/beam
median 1.3309e-04 Jy/beam
sigma 8.8073e-05 Jy/beam
MAD rms 1.0503e-05 Jy/beam

RMS images

VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms

VLASS1.2.ql.T18t10.J065626_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_T18t10.J065626+293000_P41891v1_2019_05_12T19_55_59.620/working/VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t10.J065626+293000_P41891v1_2019_05_12T19_55_59.620/working
Start time
2019-05-15 09:17:30.775
End
2019-05-15 09:19:28.913
Duration
0:01:58.138
Note, WebLog generation is not included in the time.

CASA logs for stage 6