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 6.6029e-04 Jy/beam
minimum 1.2311e-04 Jy/beam
mean 1.9074e-04 Jy/beam
median 1.5118e-04 Jy/beam
sigma 8.2032e-05 Jy/beam
MAD rms 1.8545e-05 Jy/beam

RMS images

VLASS1.2.sb36583628.eb36658350.58618.138462766205_split.ms

VLASS1.2.ql.T12t20.J130611_073000.10.2048.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_T12t20.J130611+073000_P50003v1_2019_05_28T21_37_23.308/working/VLASS1.2.sb36583628.eb36658350.58618.138462766205_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T12t20.J130611+073000_P50003v1_2019_05_28T21_37_23.308/working
Start time
2019-05-30 11:42:39.278
End
2019-05-30 11:44:56.890
Duration
0:02:17.612
Note, WebLog generation is not included in the time.

CASA logs for stage 6