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 6.0524e-04 Jy/beam
minimum 1.0974e-04 Jy/beam
mean 1.7936e-04 Jy/beam
median 1.3943e-04 Jy/beam
sigma 8.3622e-05 Jy/beam
MAD rms 2.4040e-05 Jy/beam

RMS images

VLASS1.2.sb36491285.eb36526783.58570.391316724534_split.ms

VLASS1.2.ql.T21t16.J155539_413000.10.2048.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_T21t16.J155539+413000_P39377v1_2019_10_21T22_01_56.952/working/VLASS1.2.sb36491285.eb36526783.58570.391316724534_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t16.J155539+413000_P39377v1_2019_10_21T22_01_56.952/working
Start time
2019-10-23 06:57:52.386
End
2019-10-23 06:59:56.591
Duration
0:02:04.205
Note, WebLog generation is not included in the time.

CASA logs for stage 6