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 6.4209e-04 Jy/beam
minimum 1.1296e-04 Jy/beam
mean 1.8002e-04 Jy/beam
median 1.3682e-04 Jy/beam
sigma 8.4953e-05 Jy/beam
MAD rms 1.6385e-05 Jy/beam

RMS images

VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms

VLASS1.2.ql.T18t04.J024426_283000.10.2048.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_T18t04.J024426+283000_P37835v1_2019_04_01T22_27_05.563/working/VLASS1.2.sb36468917.eb36521861.58568.73382162037_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t04.J024426+283000_P37835v1_2019_04_01T22_27_05.563/working
Start time
2019-04-03 10:29:51.751
End
2019-04-03 10:31:42.754
Duration
0:01:51.004
Note, WebLog generation is not included in the time.

CASA logs for stage 6