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 6.4524e-04 Jy/beam
minimum 1.2184e-04 Jy/beam
mean 1.9522e-04 Jy/beam
median 1.4817e-04 Jy/beam
sigma 9.6248e-05 Jy/beam
MAD rms 1.6091e-05 Jy/beam

RMS images

VLASS1.2.sb36458312.eb36595350.58593.54284034722_split.ms

VLASS1.2.ql.T20t03.J015400_393000.10.2048.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_T20t03.J015400+393000_P44878v1_2019_05_09T14_34_48.003/working/VLASS1.2.sb36458312.eb36595350.58593.54284034722_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t03.J015400+393000_P44878v1_2019_05_09T14_34_48.003/working
Start time
2019-05-11 03:55:32.408
End
2019-05-11 03:57:55.801
Duration
0:02:23.392
Note, WebLog generation is not included in the time.

CASA logs for stage 6