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 6.9073e-04 Jy/beam
minimum 1.1618e-04 Jy/beam
mean 1.8224e-04 Jy/beam
median 1.3889e-04 Jy/beam
sigma 9.2547e-05 Jy/beam
MAD rms 1.2096e-05 Jy/beam

RMS images

VLASS1.2.sb36526854.eb36581717.58589.84345299768_split.ms

VLASS1.2.ql.T17t13.J092428_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_T17t13.J092428+263000_P40699v1_2019_05_01T15_05_12.873/working/VLASS1.2.sb36526854.eb36581717.58589.84345299768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t13.J092428+263000_P40699v1_2019_05_01T15_05_12.873/working
Start time
2019-05-04 12:21:30.781
End
2019-05-04 12:23:50.386
Duration
0:02:19.605
Note, WebLog generation is not included in the time.

CASA logs for stage 6