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 7.0989e-04 Jy/beam
minimum 1.1344e-04 Jy/beam
mean 1.7754e-04 Jy/beam
median 1.3414e-04 Jy/beam
sigma 9.0680e-05 Jy/beam
MAD rms 1.1576e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T17t13.J091102_253000.10.2048.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.J091102+253000_P40685v1_2019_05_01T15_04_44.655/working/VLASS1.2.sb36526854.eb36581717.58589.84345299768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t13.J091102+253000_P40685v1_2019_05_01T15_04_44.655/working
Start time
2019-05-04 11:01:10.950
End
2019-05-04 11:03:16.947
Duration
0:02:05.997
Note, WebLog generation is not included in the time.

CASA logs for stage 6