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 5.9651e-04 Jy/beam
minimum 1.0771e-04 Jy/beam
mean 1.6906e-04 Jy/beam
median 1.2938e-04 Jy/beam
sigma 8.3279e-05 Jy/beam
MAD rms 1.1082e-05 Jy/beam

RMS images

VLASS1.2.sb36439829.eb36514324.58567.4355214699_split.ms

VLASS1.2.ql.T22t22.J214804_453000.10.2048.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_T22t22.J214804+453000_P38846v1_2019_04_25T15_21_15.878/working/VLASS1.2.sb36439829.eb36514324.58567.4355214699_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T22t22.J214804+453000_P38846v1_2019_04_25T15_21_15.878/working
Start time
2019-04-29 15:24:20.506
End
2019-04-29 15:26:47.218
Duration
0:02:26.712
Note, WebLog generation is not included in the time.

CASA logs for stage 6