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 5.9296e-04 Jy/beam
minimum 1.1081e-04 Jy/beam
mean 1.7314e-04 Jy/beam
median 1.3333e-04 Jy/beam
sigma 8.2403e-05 Jy/beam
MAD rms 1.1414e-05 Jy/beam

RMS images

VLASS1.2.sb36459161.eb36630310.58605.46792393518_split.ms

VLASS1.2.ql.T24t24.J233037_543000.10.2048.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_T24t24.J233037+543000_P44347v1_2019_05_17T23_16_41.038/working/VLASS1.2.sb36459161.eb36630310.58605.46792393518_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T24t24.J233037+543000_P44347v1_2019_05_17T23_16_41.038/working
Start time
2019-05-20 09:04:19.133
End
2019-05-20 09:06:42.210
Duration
0:02:23.078
Note, WebLog generation is not included in the time.

CASA logs for stage 6